X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries

Long Ji; Shan-Shan Weng

X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries

T0 review · 0 major / 6 minor · reviewed 2026-08-11 · deepseek-v4-flash

Challenge this review Re-run · record.json Download PDF Read on arXiv ↗

Pith's one-line read This review argues that the observable behavior of accreting X-ray pulsars is ordered by two parameters, luminosity and magnetic field, acting through the geometry of the accretion flow at the neutron star's magnetic poles.

desk verdict A solid, up-to-date review of accreting X-ray pulsars that earns its place as an entry point, even though its central L-B organizing claim is more slogan than quantitative theory. read the letter →

arxiv 2412.17275 v1 pith:IQF7DF2Z submitted 2024-12-23 astro-ph.HE

Shan-Shan Weng , Long Ji This is my paper · ORCID

classification astro-ph.HE

keywords X-raypulsarsneutronstarshigh-massbinariesaccretioncolumnscyclotronresonantscatteringfeaturespolarimetrysupergiantfasttransientspulsatingultraluminoussources

verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

This review argues that the bewildering variety of accreting X-ray pulsars in high-mass X-ray binaries can be organized by just two physical numbers: the luminosity $L$ and the magnetic field $B$ of the neutron star. Near the magnetic poles, the accretion flow takes one of two forms — a tall radiation-dominated column when $L$ exceeds a critical value $L_{\rm crit}\sim 1.5\times10^{37}(B/10^{12})^{16/15}$ erg/s, and a low-lying accretion mound below it — and the switch between them is claimed to drive changes in pulse profiles, spectra, cyclotron line energies, and variability. The paper consolidates recent timing, spectral, and polarimetric observations, and compares Galactic pulsars with gamma-ray binaries and pulsating ultraluminous X-ray sources. A sympathetic reader comes away with a testable organizing scheme: measure $L$ and $B$, and the accretion geometry and its observable fingerprints follow.

What carries the argument

The load-bearing objects are the magnetospheric radius $R_m = k(\mu^4/(2GM\dot{M}^2))^{1/7}$, the co-rotation radius $R_{\rm co}$, and the critical luminosity $L_{\rm crit}$ that separates accretion columns from accretion mounds. These combine to define the geometry that determines the beam pattern (fan versus pencil), the cyclotron line energy through the $E_{\rm cyc}\approx (n/(1+z))\,11.6\,B_{12}$ keV relation, and the torques that spin the star up or down. The same framework, with the propeller and quasi-spherical settling regimes, explains low-luminosity states and extreme transients.

What would settle it

Track torque and luminosity through a full outburst of a pulsar whose field is known from its cyclotron line; if the torque does not scale as $\dot{M}^{6/7}$ implied by $R_m\propto\dot{M}^{-2/7}$, or if the pulse-profile transition occurs at a luminosity incompatible with $L_{\rm crit}$ from Eq. (8), the organizing scheme is falsified.

Watch

Extended reading notes

Core claim

The paper's central claim is stated in Section 2.3: the accretion process near the magnetic poles and its observable properties mainly depend on luminosity and magnetic field. It gathers evidence that many otherwise disparate phenomena — single-to-double pulse profile transitions, the crossing from positive to negative cyclotron-line energy versus luminosity, the appearance of spin-phase-dependent quasi-periodic oscillations, and the low polarization degree — line up with the predicted subcritical/supercritical boundary set by $L_{\rm crit}$. In the supercritical regime a radiation-dominated shock forms and X-rays escape through the column wall as a fan beam; in the subcritical regime matter decelerates by Coulomb braking or a collisionless shock, forming an accretion mound that emits a pencil beam. The review also uses the magnetospheric radius, co-rotation radius, and propeller and settling-accretion regimes to tie spin evolution and transient behavior, including Be star outbursts and supergiant fast X-ray transients, to the same two parameters.

Load-bearing premise

The whole scheme assumes that the simple formula for the magnetospheric radius, with one universal constant, holds in every accretion state from faint to super-Eddington; if that formula fails, the inferred magnetic fields and torque interpretations lose their foundation.

Editorial extensions

If this is right

Pulse profile transitions from single-peaked to double-peaked during giant outbursts become diagnostics: they mark the crossing of $L_{\rm crit}$ and thereby measure $B$.
The observed reversal from positive to negative $E_{\rm cyc}$–luminosity correlation can be used to confirm where the accretion column starts, giving a second, model-independent handle on $B$.
Torque–luminosity scaling $\dot{\nu}\propto L^b$ with $b\sim0.8$–$1.1$ during outbursts, combined with $R_m$, allows magnetic field estimates for sources without detected cyclotron lines.
The systematic deficit of X-ray polarization ($5$–$20\%$ observed versus $60$–$80\%$ predicted) shows that column radiation-transfer models are missing physics, and phase-resolved polarimetry can reveal the beam geometry.
In the same $L$–$B$ picture, pulsating ultraluminous X-ray sources appear as the high-luminosity extension of the same accretion mode, with the debate about their magnetic fields reduced to measurable quantities.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

If the $L$–$B$ dichotomy holds, the persistently low polarization observed by IXPE may imply that the accretion column is threaded by tangled or multipolar field components, not the ideal dipole assumed in the models; this can be tested with broader-band polarimetry.
The radio detection of jets in strongly magnetized accreting pulsars, although not expected from these systems, could be tied to magnetic reconnection at the magnetosphere rather than standard disk jets; monitoring radio emission across an outburst would discriminate.
The predicted 2.223 MeV neutron-capture line from spallation in the accretion flow remains undetected; upcoming MeV telescopes should target the brightest super-Eddington outbursts, where the column density is highest.
Applying the same $L_{\rm crit}$ boundary to pulsating ultraluminous X-ray sources predicts that their pulse profiles should transition from sinusoidal to more complex shapes if they cross into the supercritical regime, a testable prediction with future X-ray timing.

Share X Bluesky LinkedIn Reddit HN

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Desk Editor's Note

read the letter

Here's my take on arXiv:2412.17275. It's a review, not a research paper, and it doesn't pretend otherwise. The value is in the synthesis: a compact, current map of accreting X-ray pulsars in HMXBs, with the standard physics (magnetospheric radius, critical luminosity, accretion columns, CRSFs, pulse profiles) laid out cleanly and the recent IXPE polarization results folded in. If I were pointing a new student at this field, this would be on the short list alongside Mushtukov & Tsygankov and the other cited reviews.

The physics is standard and accurately relayed. The formulas are the usual ones, and the paper is honest about uncertainties — e.g., the wind-fed/SFXT accretion debate, the unsettled PULX magnetic field question, and the fact that observed IXPE polarization (5–20%) is far below what all current models predict (60–80%). That last point is actually a sign of careful reviewing: it flags a real tension rather than papering over it.

Soft spots. The central organizing claim in Section 2.3 — that observable properties near the poles depend mainly on L and B — is a reasonable organizing slogan, but the paper's own content shows it's not the whole story. The polarization deficit and the PULX/Galactic AXRP differences both suggest geometry, accretion mode, and possibly mass accretion rate carry independent weight. For a review this is not fatal, and the paper does mention caveats, but the framing would be more honest if it said 'working approximation' rather than implying consensus. A referee could ask for a sentence or two of scope clarification.

Editorially, there are typos (Lcirt, magneta), duplicate references, and the MDPI layout placeholders. None of this affects the science.

Bottom line: this is a competent, useful review with no new results and no serious technical errors. It deserves peer review; a good referee will mainly help with framing and clean-up. I'd accept it after minor revision, and I'd cite it as a reference in my own writing if I needed to point someone to the current state of AXRP observations.

Referee Report

0 major / 6 minor

Summary. This review synthesizes the current understanding of accreting X-ray pulsars in high-mass X-ray binaries, covering the standard accretion physics (magnetospheric radius, propeller and settling regimes, critical luminosity), the phenomenology of outbursts and long-term variability, spin evolution, aperiodic variability, spectral formation including cyclotron lines, and the recent IXPE polarimetry results. It concludes with short discussions of gamma-ray binaries and pulsating ultraluminous X-ray sources, and of multi-wavelength advances. The paper does not claim new original analysis; its purpose is to organize and present the established literature, with emphasis on results from the last few years (Insight-HXMT, NICER, IXPE, AstroSat, Swift).

Significance. If taken as a field map, this review is largely successful and useful. Its strengths are the up-to-date selection of topics, the carefully reproduced figures (Corbet diagram, pulse-profile evolution, the E_cyc versus luminosity relation for 1A 0535+262), the concise explanations of formulas such as the magnetospheric radius and critical luminosity, and its candid reporting of open problems, notably the discrepancy between predicted and measured X-ray polarization and the unresolved magnetic-field question for PULXs. The extensive reference list provides good entry points. Because it is a review, there are no machine-checked proofs or reproducible codes to assess, but the cited physics is standard and internally consistent.

minor comments (6)

[Section 2.3 (and Sections 5, 6)] The sentence 'It is believed that the accretion process near magnetic poles and its observable properties mainly depend on the luminosity (L) and the magnetic field (B)' is stated without qualification. Sections 5 and 6 of the paper itself show that this reduction is incomplete: measured polarization degrees of 5-20% are far below the 60-80% predicted by 'all existing theoretical models', and PULXs differ from Galactic AXRPs in spectral shape and pulse profile even though both are thought to be governed by the same L and B parameters. Please add an explicit caveat that L and B are the primary, but not sufficient, determinants, and that accretion geometry and radiative transfer introduce additional degrees of freedom.
[Equation (8), Section 2.3] The symbol Lcirt appears to be a typo for Lcrit; the same misspelling recurs in Sections 3.1.1 and the footnote, and should be corrected throughout.
[Figure 1 caption] The word 'magneta' should be 'magenta'.
[Section 2.1, Equation (3) context] There is a missing space in 'andk ~ 0.5' in the sentence 'Typically,k is assumed'; also the inline equation for the accretion radius would benefit from a separating comma before the approximation sign.
[References] Reference [216] duplicates reference [116] (both are Wilson-Hodge et al., ApJ 863, 9, 2018), and reference [233] duplicates reference [232]; these should be merged to avoid inflation of the bibliography.
[Section 6] The phrase 'PULXs share s similar spin-up trend' contains a stray 's'; it should read 'share a similar spin-up trend'.

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity: the review relays externally grounded results and derives no fitted predictions from its own inputs.

full rationale

This paper is a review, not a derivation. Its central statements, such as the claim in Section 2.3 that accretion near the magnetic poles and its observable properties mainly depend on luminosity and magnetic field, are presented as a summary of a research consensus and are not derived from any quantity fitted in the paper. The magnetospheric radius, critical luminosity, and torque formulas are quoted from prior literature with explicit citations to independent theoretical and observational work, and the review does not fit parameters or make predictions that reduce to its own inputs. Where the paper cites the authors' own previous studies (e.g., Weng et al. 2017; Hou et al. 2022; Ji et al. 2021; Wang et al. 2022), those citations report specific observational or data-analysis results that are externally checkable, and they are not used as a load-bearing uniqueness theorem or as a substitute for an argument. The paper even highlights a case where theory and observation disagree, namely that measured IXPE polarization degrees of 5-20% are far below the 60-80% predicted by all existing theoretical models, which explicitly prevents the review's organizing framework from being circularly confirmed by observations. No equation in the paper is equivalent by construction to another equation, and no fitted parameter is renamed as a prediction. The review is self-contained relative to the external literature it summarizes, so no circularity is present.

Assumptions & free parameters 0 free parameters · 2 assumptions · 0 invented entities

This is a review paper, so there are no new free parameters or invented entities. The central summary relies on standard astrophysical models from the cited literature, specifically the magnetospheric radius and critical luminosity formulas.

assumptions (2)

domain assumption Magnetospheric radius model (Eq. 3): Rm = k (mu^4/(2 GM Mdot^2))^(1/7) with k ~ 0.5 for disk and ~1 for spherical accretion.
Used throughout Sections 2.2 and 3 to interpret accretion regimes and estimate magnetic fields; taken from Ghosh & Lamb (1979) and Davidson & Ostriker (1973).
domain assumption Critical luminosity formula (Eq. 8): L_crit ~ 1.5e37 (B/1e12)^(16/15) erg/s.
Used in Sections 2.3, 3.2 and 4.2 to separate sub-critical and super-critical accretion regimes; based on Basko & Sunyaev (1976) and Mushtukov et al. (2015).

how reviews work

0 comments

Cite this review

Pith. "Pith review of X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries." pith.science (2026). https://pith.science/paper/IQF7DF2Z

@misc{pith2026241217275,
  author       = {Pith},
  title        = {Pith review of: X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/IQF7DF2Z}},
  note         = {Machine review of arXiv:2412.17275}
}

abstract

Accreting X-ray pulsars, located in X-ray binaries, are neutron stars with magnetic fields as strong as $B\sim10^{12\text{--}13}$ G. This review offers a concise overview of the accretion and radiation processes of X-ray pulsars and summarizes their rich observational features, particularly focusing on complex and variable temporal phenomena, spectral properties, and evolution, the new window for X-ray polarimetry and multi-wavelength advances. We also briefly discuss other related systems, i.e., gamma-ray binaries and pulsating ultraluminous X-ray sources.

Figures

Figures reproduced from arXiv: 2412.17275 by the authors.

**Figure 1.** Corbet diagram. BeXBs in the Galaxy and Magellanic Clouds are marked with black and grey circles. The wind−fed SGXBs, disk−fed SGXBs, SFXTs, PULXs are presented with green, red, magneta, and blue symbols, respectively. Data were adopted from [18,23–27] and the references therein. Unlike low-magnetic-field NS and BH accreting systems, the accreting processes in AXRPs are influenced not only by the accretion rate but … view at source ↗

**Figure 2.** (Left) long-term lightvcurve of Swift J0243.6+6124 observed with Insight-HXMT, where color shadows present different accretion states. Middle: The evolution of pulse profiles, where transitions from the sub- to supercritical regimes and from the gas-pressure-dominated (GPD) to radiation-pressure-dominated (RPD) states are marked with red dashed lines. (Right) The color shows the evolution of power spectra with lumin… view at source ↗

**Figure 3.** A sketch showing the distinct geometries and radiation patterns for the accretion mound at low accretion rates (middle) and the accretion column at high accretion rates (right). The left panel shows a zoom-in plot of the surface of the neutron star in the case of the accretion mound. The blue arrow indicates the magnetic field direction at the pole. The arrows on the rightmost side are the legend, i.e., black arrows… view at source ↗

Figures from the paper (4 more)

**Figure 4.** Figure 4: Pulse profiles of 1A 0535+262 plotted as a function of photon energy. From left to right, the three panels show the observations made at the peak luminosity (LX > Lcrit), around Lcrit, and low luminosity (LX < Lcrit), respectively. The color bar displays the normalized…

**Figure 5.** Figure 5: Psuper – Porb diagram for different types of HMXBs and PULXs. The period values of BeXBs (black circles) were adopted from (Rajoelimanana et al. [197], Chen et al. [199] and the references therein), while data on wind accretion SGXBs (green pentagram) and RLO systems (…

**Figure 6.** Figure 6: Representative spectra of AXRPs at high- and low-luminosity states. The structure around 45 keV is caused by the cyclotron line. This plot was reproduced using the data from Tsygankov et al. [219]. 4.2. Cyclotron Resonant Scattering Features In many AXRPs, there are br…

**Figure 7.** Figure 7: The evolution of Ecyc as a function of luminosity (L) observed in 1A 0535+262. Red triangles and blue points present the data from the rising and fading phases of the 2020 giant outburst. Their discrepancy reflects the hysteresis effect. The black dashed line represent…

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

Physics of Strong Magnetism with eXTP
astro-ph.HE 2025-06 unverdicted novelty 3.0 of 10

The eXTP mission's planned instruments would enable more sensitive X-ray polarization and timing observations of magnetars and accreting pulsars, potentially testing vacuum birefringence and probing magnetic field structures.

Reference graph

Works this paper leans on

298 extracted references · 27 canonical work pages · cited by 1 Pith paper

[1]

Evidence for x Rays From Sources Outside the Solar System

Giacconi, R.; Gursky, H.; Paolini, F.R.; Rossi, B.B. Evidence for x Rays From Sources Outside the Solar System. Phys. Rev. Lett. 1962, 9, 439–443. https://doi.org/10.1103/PhysRevLett.9.439

doi:10.1103/physrevlett.9.439 1962
[2]

X-Ray Binaries

Casares, J.; Jonker, P .G.; Israelian, G. X-Ray Binaries. InHandbook of Supernovae; Alsabti, A.W.; Murdin, P ., Eds.; 2017; p. 1499. https://doi.org/10.1007/978-3-319-21846-5_111

work page doi:10.1007/978-3-319-21846-5_111 2017
[3]

Accreting Binaries; Nature, formation, and evolution; 2022

Chaty, S. Accreting Binaries; Nature, formation, and evolution; 2022. https://doi.org/10.1088/2514-3433/ac595f

doi:10.1088/2514-3433/ac595f 2022
[4]

The Milky Way in X-rays for an outside observer

Grimm, H.J.; Gilfanov, M.; Sunyaev, R. The Milky Way in X-rays for an outside observer. Log(N)-Log(S) and luminosity function of X-ray binaries from RXTE/ASM data. Astron. Astrophys. 2002, 391, 923–944, [arXiv:astro-ph/astro-ph/0109239]. https://doi.org/10.1051/0004-6361:20020826

arXiv 2002
[5]

BlackCAT: A catalogue of stellar-mass black holes in X-ray transients

Corral-Santana, J.M.; Casares, J.; Muñoz-Darias, T.; Bauer, F.E.; Martínez-Pais, I.G.; Russell, D.M. BlackCAT: A catalogue of stellar-mass black holes in X-ray transients. Astron. Astrophys. 2016, 587, A61, [arXiv:astro-ph.HE/1510.08869]. https: //doi.org/10.1051/0004-6361/201527130

arXiv 2016
[6]

X-Ray Properties of Black-Hole Binaries

Remillard, R.A.; McClintock, J.E. X-Ray Properties of Black-Hole Binaries. Annu. Rev. Astron. Astrophys. 2006, 44, 49–92, [arXiv:astro-ph/astro-ph/0606352]. https://doi.org/10.1146/annurev.astro.44.051905.092532

arXiv 2006
[7]

Modelling the behaviour of accretion flows in X-ray binaries

Done, C.; Gierli ´ nski, M.; Kubota, A. Modelling the behaviour of accretion flows in X-ray binaries. Everything you always wanted to know about accretion but were afraid to ask. Astron. Astrophys. Rev. 2007, 15, 1–66, [arXiv:astro-ph/0708.0148]. https://doi.org/10.1007/s00159-007-0006-1

arXiv 2007
[8]

Low-Mass X-ray Binaries

Bahramian, A.; Degenaar, N. Low-Mass X-ray Binaries. In Handbook of X-ray and Gamma-ray Astrophysics ; 2023; p. 120. https://doi.org/10.1007/978-981-16-4544-0_94-1

doi:10.1007/978-981-16-4544-0_94-1 2023

Show all 298 references

[9]

Low Magnetic-Field Neutron Stars in X-ray Binaries

Di Salvo, T.; Papitto, A.; Marino, A.; Iaria, R.; Burderi, L. Low Magnetic-Field Neutron Stars in X-ray Binaries. arXiv e-prints 2023, p. arXiv:2311.12516, [arXiv:astro-ph.HE/2311.12516]. https://doi.org/10.48550/arXiv.2311.12516

2023 doi arXiv
[10]

SXP 1062, a young Be X-ray binary pulsar with long spin period

Haberl, F.; Sturm, R.; Filipovi´ c, M.D.; Pietsch, W.; Crawford, E.J. SXP 1062, a young Be X-ray binary pulsar with long spin period. Implications for the neutron star birth spin. Astron. Astrophys. 2012, 537, L1, [arXiv:astro-ph.HE/1112.0491]. https: //doi.org/10.1051/0004-63...

2012 arXiv
[11]

S., I.; Gruendl, R.A.; Reyes- Iturbide, J

Hénault-Brunet, V .; Oskinova, L.M.; Guerrero, M.A.; Sun, W.; Chu, Y.H.; Evans, C.J.; Gallagher, J. S., I.; Gruendl, R.A.; Reyes- Iturbide, J. Discovery of a Be/X-ray pulsar binary and associated supernova remnant in the Wing of the Small Magellanic Cloud. Mon. Not. R. Astron....

2012 arXiv
[12]

Discovery of a putative supernova remnant around the long-period X-ray pulsar SXP 1323 in the Small Magellanic Cloud

Gvaramadze, V .V .; Kniazev, A.Y.; Oskinova, L.M. Discovery of a putative supernova remnant around the long-period X-ray pulsar SXP 1323 in the Small Magellanic Cloud. Mon. Not. R. Astron. Soc. 2019, 485, L6–L10, [arXiv:astro-ph.SR/1902.02351]. https://doi.org/10.1093/mnrasl/slz018

2019 arXiv
[13]

XMMU J050722.1-684758: discovery of a new Be X-ray binary pulsar likely associated with the supernova remnant MCSNR J0507-6847

Maitra, C.; Haberl, F.; Maggi, P .; Kavanagh, P .J.; Vasilopoulos, G.; Sasaki, M.; Filipovi´ c, M.D.; Udalski, A. XMMU J050722.1-684758: discovery of a new Be X-ray binary pulsar likely associated with the supernova remnant MCSNR J0507-6847. Mon. Not. R. Astron. Soc. 2021, 504...

2021 arXiv
[14]

Catalogue of high-mass X-ray binaries in the Galaxy (4th edition)

Liu, Q.Z.; van Paradijs, J.; van den Heuvel, E.P .J. Catalogue of high-mass X-ray binaries in the Galaxy (4th edition). Astron. Astrophys. 2006, 455, 1165–1168, [arXiv:astro-ph/0707.0549]. https://doi.org/10.1051/0004-6361:20064987

2006 arXiv
[15]

XRBcats: Galactic High Mass X-ray Binary Catalogue ⋆

Neumann, M.; Avakyan, A.; Doroshenko, V .; Santangelo, A. XRBcats: Galactic High Mass X-ray Binary Catalogue ⋆. Astron. Astrophys. 2023, 677, A134, [arXiv:astro-ph.HE/2303.16137]. https://doi.org/10.1051/0004-6361/202245728

2023 arXiv
[16]

Populations of X-Ray Sources in Galaxies

Fabbiano, G. Populations of X-Ray Sources in Galaxies. Annu. Rev. Astron. Astrophys. 2006, 44, 323–366, [arXiv:astro-ph/astro- ph/0511481]. https://doi.org/10.1146/annurev.astro.44.051905.092519

2006
[17]

Ultraluminous X-Ray Sources.Annu

Kaaret, P .; Feng, H.; Roberts, T.P . Ultraluminous X-Ray Sources.Annu. Rev. Astron. Astrophys. 2017, 55, 303–341, [arXiv:astro- ph.HE/1703.10728]. https://doi.org/10.1146/annurev-astro-091916-055259

2017 arXiv
[18]

Ultraluminous X-ray sources

King, A.; Lasota, J.P .; Middleton, M. Ultraluminous X-ray sources. New Astron. Rev. 2023, 96, 101672, [arXiv:astro- ph.HE/2302.10605]. https://doi.org/10.1016/j.newar.2022.101672

2023 arXiv
[19]

High-mass X-ray binaries as a star formation rate indicator in distant galaxies

Grimm, H.J.; Gilfanov, M.; Sunyaev, R. High-mass X-ray binaries as a star formation rate indicator in distant galaxies. Mon. Not. R. Astron. Soc. 2003, 339, 793–809, [arXiv:astro-ph/astro-ph/0205371]. https://doi.org/10.1046/j.1365-8711.2003.06224.x

2003 arXiv
[20]

X-ray emission from star-forming galaxies - I

Mineo, S.; Gilfanov, M.; Sunyaev, R. X-ray emission from star-forming galaxies - I. High-mass X-ray binaries. Mon. Not. R. Astron. Soc. 2012, 419, 2095–2115, [arXiv:astro-ph.HE/1105.4610]. https://doi.org/10.1111/j.1365-2966.2011.19862.x

2012 arXiv
[21]

Optical Analysis and Modeling of HD96670, a New Black Hole X-Ray Binary Candidate

Gomez, S.; Grindlay, J.E. Optical Analysis and Modeling of HD96670, a New Black Hole X-Ray Binary Candidate. Astrophys. J. 2021, 913, 48, [arXiv:astro-ph.HE/2211.04518]. https://doi.org/10.3847/1538-4357/abf24c

2021 arXiv
[22]

The three types of high-mass X-ray pulsator

Corbet, R.H.D. The three types of high-mass X-ray pulsator. Mon. Not. R. Astron. Soc. 1986, 220, 1047–1056. https: //doi.org/10.1093/mnras/220.4.1047

1986 doi
[23]

High-mass X-ray binaries in the Magellanic Clouds.Astron

Liu, Q.Z.; van Paradijs, J.; van den Heuvel, E.P .J. High-mass X-ray binaries in the Magellanic Clouds.Astron. Astrophys. 2005, 442, 1135–1138. https://doi.org/10.1051/0004-6361:20053718. Universe 2024, 0, 0 21 of 34

2005 doi
[24]

Spin period change and the magnetic fields of neutron stars in Be X-ray binaries in the Small Magellanic Cloud

Klus, H.; Ho, W.C.G.; Coe, M.J.; Corbet, R.H.D.; Townsend, L.J. Spin period change and the magnetic fields of neutron stars in Be X-ray binaries in the Small Magellanic Cloud. Mon. Not. R. Astron. Soc. 2014, 437, 3863–3882, [arXiv:astro-ph.SR/1311.4343]. https://doi.org/10.109...

2014 arXiv
[25]

Radio pulsations from a neutron star within the gamma-ray binary LS I +61◦ 303

Weng, S.S.; Qian, L.; Wang, B.J.; Torres, D.F.; Papitto, A.; Jiang, P .; Xu, R.; Li, J.; Yan, J.Z.; Liu, Q.Z.; et al. Radio pulsations from a neutron star within the gamma-ray binary LS I +61◦ 303. Nature Astronomy 2022, 6, 698–702, [arXiv:astro-ph.HE/2203.09423]. https://doi....

2022 arXiv
[26]

Fan-beamed X-Ray Emission from 1 to above 130 keV from the Ultraluminous X-Ray Pulsar RX J0209.6-7427 in the Small Magellanic Cloud

Hou, X.; Ge, M.Y.; Ji, L.; Zhang, S.N.; You, Y.; Tao, L.; Zhang, S.; Soria, R.; Feng, H.; Zhou, M.; et al. Fan-beamed X-Ray Emission from 1 to above 130 keV from the Ultraluminous X-Ray Pulsar RX J0209.6-7427 in the Small Magellanic Cloud. Astrophys. J. 2022, 938, 149, [arXiv:...

2022 arXiv
[27]

A catalogue of high-mass X-ray binaries in the Galaxy: from the INTEGRAL to the Gaia era

Fortin, F.; García, F.; Simaz Bunzel, A.; Chaty, S. A catalogue of high-mass X-ray binaries in the Galaxy: from the INTEGRAL to the Gaia era. Astron. Astrophys. 2023, 671, A149, [arXiv:astro-ph.HE/2302.02656]. https://doi.org/10.1051/0004-6361/202245236

2023 arXiv
[28]

Be/X-ray binaries

Reig, P . Be/X-ray binaries. Astrophys. Space Sci. 2011, 332, 1–29, [arXiv:astro-ph.HE/1101.5036]. https://doi.org/10.1007/s10509 -010-0575-8

2011 arXiv
[29]

X-ray pulsars: a review

Caballero, I.; Wilms, J. X-ray pulsars: a review. Mem. Soc. Astron. Italiana 2012, 83, 230, [arXiv:astro-ph.HE/1206.3124]. https://doi.org/10.48550/arXiv.1206.3124

2012 doi arXiv
[30]

High-mass X-ray binaries in the Milky Way

Walter, R.; Lutovinov, A.A.; Bozzo, E.; Tsygankov, S.S. High-mass X-ray binaries in the Milky Way. A closer look with INTEGRAL. Astron. Astrophys. Rev. 2015, 23, 2, [arXiv:astro-ph.HE/1505.03651]. https://doi.org/10.1007/s00159-015-0082-6

2015 arXiv
[31]

Cyclotron lines in highly magnetized neutron stars

Staubert, R.; Trümper, J.; Kendziorra, E.; Klochkov, D.; Postnov, K.; Kretschmar, P .; Pottschmidt, K.; Haberl, F.; Rothschild, R.E.; Santangelo, A.; et al. Cyclotron lines in highly magnetized neutron stars. Astron. Astrophys. 2019, 622, A61, [arXiv:astro- ph.HE/1812.03461]. ...

2019 arXiv
[32]

Advances in Understanding High-Mass X-ray Binaries with INTEGRALand Future Directions

Kretschmar, P .; Fürst, F.; Sidoli, L.; Bozzo, E.; Alfonso-Garzón, J.; Bodaghee, A.; Chaty, S.; Chernyakova, M.; Ferrigno, C.; Manousakis, A.; et al. Advances in Understanding High-Mass X-ray Binaries with INTEGRALand Future Directions. New Astron. Rev. 2019, 86, 101546, [arXi...

2019 arXiv
[33]

Accreting strongly magnetised neutron stars: X-ray Pulsars.arXiv e-prints 2022, p

Mushtukov, A.; Tsygankov, S. Accreting strongly magnetised neutron stars: X-ray Pulsars.arXiv e-prints 2022, p. arXiv:2204.14185, [arXiv:astro-ph.HE/2204.14185]. https://doi.org/10.48550/arXiv.2204.14185

2022 doi arXiv
[34]

High-mass X-ray Binaries

Fornasini, F.M.; Antoniou, V .; Dubus, G. High-mass X-ray Binaries. arXiv e-prints 2023, p. arXiv:2308.02645, [arXiv:astro- ph.HE/2308.02645]. https://doi.org/10.48550/arXiv.2308.02645

2023 doi arXiv
[35]

The Imaging X-Ray Polarimetry Explorer (IXPE): Pre-Launch

Weisskopf, M.C.; Soffitta, P .; Baldini, L.; Ramsey, B.D.; O’Dell, S.L.; Romani, R.W.; Matt, G.; Deininger, W.D.; Baumgartner, W.H.; Bellazzini, R.; et al. The Imaging X-Ray Polarimetry Explorer (IXPE): Pre-Launch. Journal of Astronomical Telescopes, Instruments, and Systems 2...

2022 arXiv
[36]

X-ray Polarimetry of X-ray Pulsars

Poutanen, J.; Tsygankov, S.S.; Forsblom, S.V . X-ray Polarimetry of X-ray Pulsars. Galaxies 2024, 12, 46, [arXiv:astro- ph.HE/2408.04431]. https://doi.org/10.3390/galaxies12040046

2024 arXiv
[37]

The Fourth IBIS/ISGRI Soft Gamma-ray Survey Catalog

Bird, A.J.; Bazzano, A.; Bassani, L.; Capitanio, F.; Fiocchi, M.; Hill, A.B.; Malizia, A.; McBride, V .A.; Scaringi, S.; Sguera, V .; et al. The Fourth IBIS/ISGRI Soft Gamma-ray Survey Catalog. Astrophys. J. Suppl. Ser. 2010, 186, 1–9, [arXiv:astro-ph.HE/0910.1704]. https://do...

2010 arXiv
[38]

High-mass X-ray binaries in the Small Magellanic Cloud

Haberl, F.; Sturm, R. High-mass X-ray binaries in the Small Magellanic Cloud. Astron. Astrophys. 2016, 586, A81, [arXiv:astro- ph.GA/1511.00445]. https://doi.org/10.1051/0004-6361/201527326

2016 arXiv
[39]

Observations of Accreting Pulsars

Bildsten, L.; Chakrabarty, D.; Chiu, J.; Finger, M.H.; Koh, D.T.; Nelson, R.W.; Prince, T.A.; Rubin, B.C.; Scott, D.M.; Stollberg, M.; et al. Observations of Accreting Pulsars. Astrophys. J. Suppl. Ser. 1997, 113, 367–408, [arXiv:astro-ph/astro-ph/9707125]. https://doi.org/10....

1997 arXiv
[40]

The Ups and Downs of Accreting X-Ray Pulsars: Decade-long Observations with the Fermi Gamma-Ray Burst Monitor.Astrophys

Malacaria, C.; Jenke, P .; Roberts, O.J.; Wilson-Hodge, C.A.; Cleveland, W.H.; Mailyan, B.; GBM Accreting Pulsars Program Team. The Ups and Downs of Accreting X-Ray Pulsars: Decade-long Observations with the Fermi Gamma-Ray Burst Monitor.Astrophys. J. 2020, 896, 90. https://do...

2020 doi
[41]

Formation and evolution of compact stellar X-ray sources

Tauris, T.M.; van den Heuvel, E.P .J. Formation and evolution of compact stellar X-ray sources. InCompact stellar X-ray sources; Lewin, W.H.G.; van der Klis, M., Eds.; 2006; Vol. 39, pp. 623–665. https://doi.org/10.48550/arXiv.astro-ph/0303456

2006 doi arXiv
[42]

The Formation and Evolution of Relativistic Binaries

van den Heuvel, E.P .J. The Formation and Evolution of Relativistic Binaries. In Proceedings of the Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence; Colpi, M.; Casella, P .; Gorini, V .; Moschella, U.; Possenti, A., Eds., 2009, Vol. 359, Astrophy...

2009 doi
[43]

Nature, Formation, and Evolution of High Mass X-Ray Binaries

Chaty, S. Nature, Formation, and Evolution of High Mass X-Ray Binaries. In Proceedings of the Evolution of Compact Binaries; Schmidtobreick, L.; Schreiber, M.R.; Tappert, C., Eds., 2011, Vol. 447, Astronomical Society of the Pacific Conference Series, p. 29, [arXiv:astro-ph.HE...

2011 doi arXiv
[44]

Formation of Double Neutron Star Systems

Tauris, T.M.; Kramer, M.; Freire, P .C.C.; Wex, N.; Janka, H.T.; Langer, N.; Podsiadlowski, P .; Bozzo, E.; Chaty, S.; Kruckow, M.U.; et al. Formation of Double Neutron Star Systems. Astrophys. J. 2017, 846, 170, [arXiv:astro-ph.HE/1706.09438]. https: //doi.org/10.3847/1538-43...

2017 arXiv
[45]

Be X-ray binaries in the SMC as indicators of mass-transfer efficiency

Vinciguerra, S.; Neijssel, C.J.; Vigna-Gómez, A.; Mandel, I.; Podsiadlowski, P .; Maccarone, T.J.; Nicholl, M.; Kingdon, S.; Perry, A.; Salemi, F. Be X-ray binaries in the SMC as indicators of mass-transfer efficiency. Mon. Not. R. Astron. Soc. 2020, 498, 4705–4720, [arXiv:ast...

2020 arXiv
[46]

Radiation-driven winds in Of stars

Castor, J.I.; Abbott, D.C.; Klein, R.I. Radiation-driven winds in Of stars. Astrophys. J. 1975, 195, 157–174. https://doi.org/10.108 6/153315. Universe 2024, 0, 0 22 of 34

1975
[47]

A natural explanation for periodic X-ray outbursts in Be/X-ray binaries

Okazaki, A.T.; Negueruela, I. A natural explanation for periodic X-ray outbursts in Be/X-ray binaries. Astron. Astrophys. 2001, 377, 161–174, [arXiv:astro-ph/astro-ph/0108037]. https://doi.org/10.1051/0004-6361:20011083

2001 arXiv
[48]

Are There Magnetars in High-Mass X-Ray Binaries? The Case of Supergiant Fast X-Ray Transients

Bozzo, E.; Falanga, M.; Stella, L. Are There Magnetars in High-Mass X-Ray Binaries? The Case of Supergiant Fast X-Ray Transients. Astrophys. J. 2008, 683, 1031–1044, [arXiv:astro-ph/0805.1849]. https://doi.org/10.1086/589990

2008 arXiv
[49]

Physics of strongly magnetized neutron stars

Harding, A.K.; Lai, D. Physics of strongly magnetized neutron stars. Reports on Progress in Physics 2006, 69, 2631–2708, [arXiv:astro-ph/astro-ph/0606674]. https://doi.org/10.1088/0034-4885/69/9/R03

2006 arXiv
[50]

The limiting luminosity of accreting neutron stars with magnetic fields

Basko, M.M.; Sunyaev, R.A. The limiting luminosity of accreting neutron stars with magnetic fields. Mon. Not. R. Astron. Soc. 1976, 175, 395–417. https://doi.org/10.1093/mnras/175.2.395

1976 doi
[51]

Thermal and Bulk Comptonization in Accretion-powered X-Ray Pulsars.Astrophys

Becker, P .A.; Wolff, M.T. Thermal and Bulk Comptonization in Accretion-powered X-Ray Pulsars.Astrophys. J. 2007, 654, 435–457, [arXiv:astro-ph/astro-ph/0609035]. https://doi.org/10.1086/509108

2007 arXiv
[52]

Spectral formation in accreting X-ray pulsars: bimodal variation of the cyclotron energy with luminosity

Becker, P .A.; Klochkov, D.; Schönherr, G.; Nishimura, O.; Ferrigno, C.; Caballero, I.; Kretschmar, P .; Wolff, M.T.; Wilms, J.; Staubert, R. Spectral formation in accreting X-ray pulsars: bimodal variation of the cyclotron energy with luminosity. Astron. Astrophys. 2012, 544,...

2012 arXiv
[53]

The critical accretion luminosity for magnetized neutron stars

Mushtukov, A.A.; Suleimanov, V .F.; Tsygankov, S.S.; Poutanen, J. The critical accretion luminosity for magnetized neutron stars. Mon. Not. R. Astron. Soc. 2015, 447, 1847–1856, [arXiv:astro-ph.HE/1409.6457]. https://doi.org/10.1093/mnras/stu2484

2015 arXiv
[54]

A Generalized Analytical Model for Thermal and Bulk Comptonization in Accretion-powered X-Ray Pulsars

Becker, P .A.; Wolff, M.T. A Generalized Analytical Model for Thermal and Bulk Comptonization in Accretion-powered X-Ray Pulsars. Astrophys. J. 2022, 939, 67. https://doi.org/10.3847/1538-4357/ac8d95

2022 doi
[55]

Evidence for Strong Cyclotron Emission in the Hard X-Ray Spectrum of Her X-1

Trümper, J.; Pietsch, W.; Reppin, C.; Sacco, B. Evidence for Strong Cyclotron Emission in the Hard X-Ray Spectrum of Her X-1. In Proceedings of the Eighth Texas Symposium on Relativistic Astrophysics; Papagiannis, M.D., Ed., 1977, Vol. 302, p. 538. https://doi.org/10.1111/j.17...

1977
[56]

Neutron-Star Accretion in a Stellar Wind: Model for a Pulsed X-Ray Source

Davidson, K.; Ostriker, J.P . Neutron-Star Accretion in a Stellar Wind: Model for a Pulsed X-Ray Source. Astrophys. J. 1973, 179, 585–598. https://doi.org/10.1086/151897

1973 doi
[57]

Accretion by rotating magnetic neutron stars

Ghosh, P .; Lamb, F.K. Accretion by rotating magnetic neutron stars. III. Accretion torques and period changes in pulsating X-ray sources. Astrophys. J. 1979, 234, 296–316. https://doi.org/10.1086/157498

1979 doi
[58]

Spindown of neutron stars in close binary systems - II

Davies, R.E.; Pringle, J.E. Spindown of neutron stars in close binary systems - II. Mon. Not. R. Astron. Soc. 1981, 196, 209–224. https://doi.org/10.1093/mnras/196.2.209

1981 doi
[59]

Theory of quasi-spherical accretion in X-ray pulsars

Shakura, N.; Postnov, K.; Kochetkova, A.; Hjalmarsdotter, L. Theory of quasi-spherical accretion in X-ray pulsars. Mon. Not. R. Astron. Soc. 2012, 420, 216–236, [arXiv:astro-ph.HE/1110.3701]. https://doi.org/10.1111/j.1365-2966.2011.20026.x

2012 arXiv
[60]

Spin Evolution of Neutron Stars

Abolmasov, P .; Biryukov, A.; Popov, S.B. Spin Evolution of Neutron Stars. Galaxies 2024, 12, 7, [arXiv:astro-ph.HE/2402.04331]. https://doi.org/10.3390/galaxies12010007

2024 arXiv
[61]

Astrophysical Implications and Observational Prospects of X-Ray Polarimetry

Meszaros, P .; Novick, R.; Szentgyorgyi, A.; Chanan, G.A.; Weisskopf, M.C. Astrophysical Implications and Observational Prospects of X-Ray Polarimetry. Astrophys. J. 1988, 324, 1056. https://doi.org/10.1086/165962

1988 doi
[62]

Polarization of accreting X-ray pulsars

Caiazzo, I.; Heyl, J. Polarization of accreting X-ray pulsars. I. A new model. Mon. Not. R. Astron. Soc. 2021, 501, 109–128, [arXiv:astro-ph.HE/2009.00631]. https://doi.org/10.1093/mnras/staa3428

2021 arXiv
[63]

Complex variations in X-ray polarization in the X-ray pulsar LS V +44 17/RX J0440.9+4431

Doroshenko, V .; Poutanen, J.; Heyl, J.; Tsygankov, S.S.; Caiazzo, I.; Turolla, R.; Veledina, A.; Weisskopf, M.C.; Forsblom, S.V .; González-Caniulef, D.; et al. Complex variations in X-ray polarization in the X-ray pulsar LS V +44 17/RX J0440.9+4431. Astron. Astrophys. 2023, ...

2023 arXiv
[64]

A new correlation for Be/X-ray binaries: the orbital period-Hα equivalent width diagram

Reig, P .; Fabregat, J.; Coe, M.J. A new correlation for Be/X-ray binaries: the orbital period-Hα equivalent width diagram. Astron. Astrophys. 1997, 322, 193–196

1997
[65]

Near IR spectroscopy of candidate B[e]/X-ray binaries.Astron

Clark, J.S.; Steele, I.A.; Fender, R.P .; Coe, M.J. Near IR spectroscopy of candidate B[e]/X-ray binaries.Astron. Astrophys. 1999, 348, 888–896

1999
[66]

Optical properties of Small Magellanic Cloud X-ray binaries.Mon

Coe, M.J.; Edge, W.R.T.; Galache, J.L.; McBride, V .A. Optical properties of Small Magellanic Cloud X-ray binaries.Mon. Not. R. Astron. Soc. 2005, 356, 502–514, [arXiv:astro-ph/astro-ph/0410074]. https://doi.org/10.1111/j.1365-2966.2004.08467.x

2005 arXiv
[67]

Optical, ultraviolet and infrared observations of X-ray binaries

Charles, P .A.; Coe, M.J. Optical, ultraviolet and infrared observations of X-ray binaries. InCompact stellar X-ray sources; Lewin, W.H.G.; van der Klis, M., Eds.; 2006; Vol. 39, pp. 215–265

2006
[68]

Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL

Chaty, S.; Rahoui, F.; Foellmi, C.; Tomsick, J.A.; Rodriguez, J.; Walter, R. Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. I. The nature of the companion star. Astron. Astrophys. 2008, 484, 783–800, [arXiv:astro- ph/0802.1774]. https://do...

2008 arXiv
[69]

Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL

Rahoui, F.; Chaty, S.; Lagage, P .O.; Pantin, E. Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. II. The environment of the companion star. Astron. Astrophys. 2008, 484, 801–813, [arXiv:astro-ph/0802.1770]. https://doi.org/10.1051/0004-6361...

2008 arXiv
[70]

A new radio census of neutron star X-ray binaries

van den Eijnden, J.; Degenaar, N.; Russell, T.D.; Wijnands, R.; Bahramian, A.; Miller-Jones, J.C.A.; Hernández Santisteban, J.V .; Gallo, E.; Atri, P .; Plotkin, R.M.; et al. A new radio census of neutron star X-ray binaries. Mon. Not. R. Astron. Soc. 2021, 507, 3899–3922, [ar...

2021 arXiv
[71]

Radiation-driven winds of hot stars

Kudritzki, R.P .; Pauldrach, A.; Puls, J.; Abbott, D.C. Radiation-driven winds of hot stars. VI. Analytical solutions for wind models including the finite cone angle effect. Astron. Astrophys. 1989, 219, 205–218

1989
[72]

Instabilities in line-driven stellar winds

Owocki, S.P .; Rybicki, G.B. Instabilities in line-driven stellar winds. I. Dependence on perturbation wavelength. Astrophys. J. 1984, 284, 337–350. https://doi.org/10.1086/162412. Universe 2024, 0, 0 23 of 34

1984 doi
[73]

Time-dependent Models of Radiatively Driven Stellar Winds

Owocki, S.P .; Castor, J.I.; Rybicki, G.B. Time-dependent Models of Radiatively Driven Stellar Winds. I. Nonlinear Evolution of Instabilities for a Pure Absorption Model. Astrophys. J. 1988, 335, 914. https://doi.org/10.1086/166977

1988 doi
[74]

The clumpy absorber in the high-mass X-ray binary Vela X-1

Grinberg, V .; Hell, N.; El Mellah, I.; Neilsen, J.; Sander, A.A.C.; Leutenegger, M.; Fürst, F.; Huenemoerder, D.P .; Kretschmar, P .; Kühnel, M.; et al. The clumpy absorber in the high-mass X-ray binary Vela X-1. Astron. Astrophys. 2017, 608, A143, [arXiv:astro-ph.HE/1711.067...

2017 arXiv
[75]

Classical Be stars

Rivinius, T.; Carciofi, A.C.; Martayan, C. Classical Be stars. Rapidly rotating B stars with viscous Keplerian decretion disks. Astron. Astrophys. Rev. 2013, 21, 69, [arXiv:astro-ph.SR/1310.3962]. https://doi.org/10.1007/s00159-013-0069-0

2013 arXiv
[76]

Origin of Two Types of X-Ray Outbursts in Be/X-Ray Binaries

Okazaki, A.T.; Hayasaki, K.; Moritani, Y. Origin of Two Types of X-Ray Outbursts in Be/X-Ray Binaries. I. Accretion Scenarios. Publ. Astron. Soc. Pac. 2013, 65, 41, [arXiv:astro-ph.HE/1211.5225]. https://doi.org/10.1093/pasj/65.2.41

2013 arXiv
[77]

Giant Outbursts in Be/X-Ray Binaries.Astrophys

Martin, R.G.; Nixon, C.; Armitage, P .J.; Lubow, S.H.; Price, D.J. Giant Outbursts in Be/X-Ray Binaries.Astrophys. J. Lett. 2014, 790, L34, [arXiv:astro-ph.HE/1407.5676]. https://doi.org/10.1088/2041-8205/790/2/L34

2014 arXiv
[78]

The origin of long-period X-ray pulsars

Ikhsanov, N.R. The origin of long-period X-ray pulsars. Mon. Not. R. Astron. Soc. 2007, 375, 698–704, [arXiv:astro-ph/astro- ph/0611442]. https://doi.org/10.1111/j.1365-2966.2006.11331.x

2007
[79]

Non-axisymmetric wind-accretion simulations

Ruffert, M. Non-axisymmetric wind-accretion simulations. II. Density gradients. Astron. Astrophys. 1999, 346, 861–877, [arXiv:astro-ph/astro-ph/9903304]. https://doi.org/10.48550/arXiv.astro-ph/9903304

1999 doi arXiv
[80]

Centrifugal barriers in magnetospheric accretion

Lyutikov, M. Centrifugal barriers in magnetospheric accretion. Mon. Not. R. Astron. Soc. 2023, 520, 4315–4323, [arXiv:astro- ph.HE/2210.00300]. https://doi.org/10.1093/mnras/stad284

2023 arXiv
[81]

The Quiescent X-Ray Emission of Three Transient X-Ray Pulsars

Campana, S.; Stella, L.; Israel, G.L.; Moretti, A.; Parmar, A.N.; Orlandini, M. The Quiescent X-Ray Emission of Three Transient X-Ray Pulsars. Astrophys. J. 2002, 580, 389–393, [arXiv:astro-ph/astro-ph/0207422]. https://doi.org/10.1086/343074

2002 arXiv
[82]

Propeller effect in two brightest transient X-ray pulsars: 4U 0115+63 and V 0332+53

Tsygankov, S.S.; Lutovinov, A.A.; Doroshenko, V .; Mushtukov, A.A.; Suleimanov, V .; Poutanen, J. Propeller effect in two brightest transient X-ray pulsars: 4U 0115+63 and V 0332+53. Astron. Astrophys. 2016, 593, A16, [arXiv:astro-ph.HE/1602.03177]. https://doi.org/10.1051/000...

2016 arXiv
[83]

Accretion by rotating magnetic neutron stars

Ghosh, P .; Lamb, F.K. Accretion by rotating magnetic neutron stars. II. Radial and vertical structure of the transition zone in disk accretion. Astrophys. J. 1979, 232, 259–276. https://doi.org/10.1086/157285

1979 doi
[84]

Disc accretion by magnetized neutron stars : a reassessment of the torque

Wang, Y.M. Disc accretion by magnetized neutron stars : a reassessment of the torque. Astron. Astrophys. 1987, 183, 257–264

1987
[85]

On the Torque Exerted by a Magnetically Threaded Accretion Disk

Wang, Y.M. On the Torque Exerted by a Magnetically Threaded Accretion Disk. Astrophys. J. Lett. 1995, 449, L153. https: //doi.org/10.1086/309649

1995 doi
[86]

Accretion onto Fast X-Ray Pulsars

Rappaport, S.A.; Fregeau, J.M.; Spruit, H. Accretion onto Fast X-Ray Pulsars. Astrophys. J. 2004, 606, 436–443, [arXiv:astro- ph/astro-ph/0310224]. https://doi.org/10.1086/382863

2004 arXiv
[87]

Magnetically Torqued Thin Accretion Disks

Klu´ zniak, W.; Rappaport, S. Magnetically Torqued Thin Accretion Disks. Astrophys. J. 2007, 671, 1990–2005, [arXiv:astro- ph/0709.2361]. https://doi.org/10.1086/522954

2007 arXiv
[88]

Super Strong Magnetic Fields of Neutron Stars in Be X-Ray Binaries Estimated with New Torque and Magnetosphere Models

Shi, C.S.; Zhang, S.N.; Li, X.D. Super Strong Magnetic Fields of Neutron Stars in Be X-Ray Binaries Estimated with New Torque and Magnetosphere Models. Astrophys. J. 2015, 813, 91, [arXiv:astro-ph.HE/1509.06126]. https://doi.org/10.1088/0004-637X/81 3/2/91

2015 arXiv
[89]

Magnetospheric radius of an inclined rotator in the magnetically threaded disk model

Bozzo, E.; Ascenzi, S.; Ducci, L.; Papitto, A.; Burderi, L.; Stella, L. Magnetospheric radius of an inclined rotator in the magnetically threaded disk model. Astron. Astrophys. 2018, 617, A126, [arXiv:astro-ph.HE/1806.11516]. https://doi.org/10.1051/0004-6361/ 201732004

2018 arXiv
[90]

Black holes in binary systems

Shakura, N.I.; Sunyaev, R.A. Black holes in binary systems. Observational appearance. Astron. Astrophys. 1973, 24, 337–355

1973
[91]

Super-Eddington accretion on to a magnetized neutron star

Chashkina, A.; Abolmasov, P .; Poutanen, J. Super-Eddington accretion on to a magnetized neutron star. Mon. Not. R. Astron. Soc. 2017, 470, 2799–2813, [arXiv:astro-ph.HE/1703.07005]. https://doi.org/10.1093/mnras/stx1372

2017 arXiv
[92]

Super-Eddington accretion discs with advection and outflows around magnetized neutron stars

Chashkina, A.; Lipunova, G.; Abolmasov, P .; Poutanen, J. Super-Eddington accretion discs with advection and outflows around magnetized neutron stars. Astron. Astrophys. 2019, 626, A18, [arXiv:astro-ph.HE/1902.04609]. https://doi.org/10.1051/0004-636 1/201834414

2019 arXiv
[93]

Hot disc of the Swift J0243.6+6124 revealed by Insight-HXMT

Doroshenko, V .; Zhang, S.N.; Santangelo, A.; Ji, L.; Tsygankov, S.; Mushtukov, A.; Qu, L.J.; Zhang, S.; Ge, M.Y.; Chen, Y.P .; et al. Hot disc of the Swift J0243.6+6124 revealed by Insight-HXMT. Mon. Not. R. Astron. Soc. 2020, 491, 1857–1867, [arXiv:astro- ph.HE/1909.12614]. ...

2020
[94]

Timing analysis of 2S 1417-624 observed with NICER and Insight-HXMT

Ji, L.; Doroshenko, V .; Santangelo, A.; Güngör, C.; Zhang, S.; Ducci, L.; Zhang, S.N.; Ge, M.Y.; Qu, L.J.; Chen, Y.P .; et al. Timing analysis of 2S 1417-624 observed with NICER and Insight-HXMT. Mon. Not. R. Astron. Soc. 2020, 491, 1851–1856, [arXiv:astro-ph.HE/1910.03955]. ...

2020
[95]

Two Complete Spectral Transitions of Swift J0243.6+6124 Observed by Insight-HXMT

Kong, L.D.; Zhang, S.; Chen, Y.P .; Zhang, S.N.; Ji, L.; Doroshenko, V .; Wang, P .J.; Tao, L.; Ge, M.Y.; Liu, C.Z.; et al. Two Complete Spectral Transitions of Swift J0243.6+6124 Observed by Insight-HXMT. Astrophys. J. 2020, 902, 18. https://doi.org/10.3847/1538 -4357/abb241

2020 doi
[96]

Evidence for the radiation- pressure dominated accretion disk in bursting pulsar GRO J1744-28 using timing analysis

Mönkkönen, J.; Tsygankov, S.S.; Mushtukov, A.A.; Doroshenko, V .; Suleimanov, V .F.; Poutanen, J. Evidence for the radiation- pressure dominated accretion disk in bursting pulsar GRO J1744-28 using timing analysis. Astron. Astrophys. 2019, 626, A106, [arXiv:astro-ph.HE/1905.05...

2019 arXiv
[97]

Super-Eddington accretion of the first Galactic ultra-luminous X-ray pulsar Swift J0243.6+6124

Liu, J.; Jenke, P .A.; Ji, L.; Zhang, S.N.; Zhang, S.; Ge, M.; Liao, J.; Li, X.; Song, L. Super-Eddington accretion of the first Galactic ultra-luminous X-ray pulsar Swift J0243.6+6124. Mon. Not. R. Astron. Soc. 2022, 512, 5686–5692. https://doi.org/10.1093/mnras/ stac836. Uni...

2022 doi
[98]

Accretion onto magnetized neutron stars - X-ray pulsars with intermediate rotation rates

Burnard, D.J.; Arons, J.; Lea, S.M. Accretion onto magnetized neutron stars - X-ray pulsars with intermediate rotation rates. Astrophys. J. 1983, 266, 175–187. https://doi.org/10.1086/160768

1983 doi
[99]

Wind accretion: Theory and observations

Shakura, N.I.; Postnov, K.A.; Kochetkova, A.Y.; Hjalmarsdotter, L.; Sidoli, L.; Paizis, A. Wind accretion: Theory and observations. Astronomy Reports 2015, 59, 645–655, [arXiv:astro-ph.HE/1407.3163]. https://doi.org/10.1134/S1063772915070112

2015 arXiv
[100]

MHD instabilities in accretion mounds - I

Mukherjee, D.; Bhattacharya, D.; Mignone, A. MHD instabilities in accretion mounds - I. 2D axisymmetric simulations. Mon. Not. R. Astron. Soc. 2013, 430, 1976–1987, [arXiv:astro-ph.HE/1212.3897]. https://doi.org/10.1093/mnras/stt020

2013 arXiv
[101]

Three-dimensional modelling of accretion columns: spatial asymmetry and self-consistent simulations

Gornostaev, M.I. Three-dimensional modelling of accretion columns: spatial asymmetry and self-consistent simulations. Mon. Not. R. Astron. Soc. 2021, 501, 564–575, [arXiv:astro-ph.HE/2012.10501]. https://doi.org/10.1093/mnras/staa3560

2021 arXiv
[102]

Radiative transfer in a strong magnetic field and accreting X-ray pulsars

Basko, M.M.; Sunyaev, R.A. Radiative transfer in a strong magnetic field and accreting X-ray pulsars. Astron. Astrophys. 1975, 42, 311–321

1975
[103]

Spin-reversed accretion as the cause of intermittent spindown in slowX-ray pulsars

Wang, Y.M. Spin-reversed accretion as the cause of intermittent spindown in slowX-ray pulsars. Astron. Astrophys. 1981, 102, 36–44

1981
[104]

On the dependence of the X-ray continuum variations with luminosity in accreting X-ray pulsars

Postnov, K.A.; Gornostaev, M.I.; Klochkov, D.; Laplace, E.; Lukin, V .V .; Shakura, N.I. On the dependence of the X-ray continuum variations with luminosity in accreting X-ray pulsars. Mon. Not. R. Astron. Soc. 2015, 452, 1601–1611, [arXiv:astro- ph.HE/1506.07082]. https://doi...

2015 arXiv
[105]

Radiative relativistic magnetohydrodynamic simulations of neutron star column accretion in Cartesian geometry

Zhang, L.; Blaes, O.; Jiang, Y.F. Radiative relativistic magnetohydrodynamic simulations of neutron star column accretion in Cartesian geometry. Mon. Not. R. Astron. Soc. 2022, 515, 4371–4390, [arXiv:astro-ph.HE/2206.13759]. https://doi.org/10.1093/ mnras/stac1815

2022 arXiv
[106]

Low-luminosity accretion onto magnetized neutron stars

Langer, S.H.; Rappaport, S. Low-luminosity accretion onto magnetized neutron stars. Astrophys. J. 1982, 257, 733–751. https://doi.org/10.1086/160028

1982 doi
[107]

X-ray emission from magnetized neutron star atmospheres at low mass-accretion rates

Sokolova-Lapa, E.; Gornostaev, M.; Wilms, J.; Ballhausen, R.; Falkner, S.; Postnov, K.; Thalhammer, P .; Fürst, F.; García, J.A.; Shakura, N.; et al. X-ray emission from magnetized neutron star atmospheres at low mass-accretion rates. I. Phase-averaged spectrum. Astron. Astrop...

2021 arXiv
[108]

Spectrum formation in X-ray pulsars at very low mass accretion rate: Monte Carlo approach

Mushtukov, A.A.; Suleimanov, V .F.; Tsygankov, S.S.; Portegies Zwart, S. Spectrum formation in X-ray pulsars at very low mass accretion rate: Monte Carlo approach. Mon. Not. R. Astron. Soc. 2021, 503, 5193–5203, [arXiv:astro-ph.HE/2006.13596]. https://doi.org/10.1093/mnras/stab811

2021 arXiv
[109]

A New Class of High-Mass X-Ray Binaries: Implications for Core Collapse and Neutron Star Recoil

Pfahl, E.; Rappaport, S.; Podsiadlowski, P .; Spruit, H. A New Class of High-Mass X-Ray Binaries: Implications for Core Collapse and Neutron Star Recoil. Astrophys. J. 2002, 574, 364–376, [arXiv:astro-ph/astro-ph/0109521]. https://doi.org/10.1086/340794

2002 arXiv
[110]

Discovery of two new persistent Be/X-ray pulsar systems

Reig, P .; Roche, P . Discovery of two new persistent Be/X-ray pulsar systems. Mon. Not. R. Astron. Soc. 1999, 306, 100–106, [arXiv:astro-ph/astro-ph/9902221]. https://doi.org/10.1046/j.1365-8711.1999.02473.x

1999 arXiv
[111]

Broad-band observations of the Be/X-ray binary pulsar RX J0440.9+4431: discovery of a cyclotron absorption line

Tsygankov, S.S.; Krivonos, R.A.; Lutovinov, A.A. Broad-band observations of the Be/X-ray binary pulsar RX J0440.9+4431: discovery of a cyclotron absorption line. Mon. Not. R. Astron. Soc. 2012, 421, 2407–2413, [arXiv:astro-ph.HE/1201.0616]. https://doi.org/10.1111/j.1365-2966....

2012 arXiv
[112]

Discovery of spin-phase-dependent QPOs in the supercritical accretion regime from the X-ray pulsar RX J0440.9+4431

Malacaria, C.; Huppenkothen, D.; Roberts, O.J.; Ducci, L.; Bozzo, E.; Jenke, P .; Wilson-Hodge, C.A.; Falanga, M. Discovery of spin-phase-dependent QPOs in the supercritical accretion regime from the X-ray pulsar RX J0440.9+4431. Astron. Astrophys. 2024, 681, A25, [arXiv:astro...

2024 arXiv
[113]

Broad-band noise and quasi-periodic oscillation characteristics of the X-ray pulsar RX J0440.9+4431

Li, P .P .; Tao, L.; Ma, R.C.; Ge, M.Y.; Zhao, Q.C.; Zhao, S.J.; Zhang, L.; Bu, Q.C.; Kong, L.D.; Tuo, Y.L.; et al. Broad-band noise and quasi-periodic oscillation characteristics of the X-ray pulsar RX J0440.9+4431. Mon. Not. R. Astron. Soc. 2024, 529, 1187–1194, [arXiv:astro...

2024 arXiv
[114]

Swift Observations of SMC X-3 during Its 2016-2017 Super-Eddington Outburst

Weng, S.S.; Ge, M.Y.; Zhao, H.H.; Wang, W.; Zhang, S.N.; Bian, W.H.; Yuan, Q.R. Swift Observations of SMC X-3 during Its 2016-2017 Super-Eddington Outburst. Astrophys. J. 2017, 843, 69, [arXiv:astro-ph.HE/1701.02983]. https://doi.org/10.3847/1538 -4357/aa76ec

2016 arXiv
[115]

Study of recent outburst in the Be/X-ray binary RX J0209.6-7427 with AstroSat: a new ultraluminous X-ray pulsar in the Magellanic Bridge? Mon

Chandra, A.D.; Roy, J.; Agrawal, P .C.; Choudhury, M. Study of recent outburst in the Be/X-ray binary RX J0209.6-7427 with AstroSat: a new ultraluminous X-ray pulsar in the Magellanic Bridge? Mon. Not. R. Astron. Soc. 2020, 495, 2664–2672, [arXiv:astro-ph.HE/2004.04930]. https...

2020 arXiv
[117]

Super-Eddington Accretion onto the Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124

Tao, L.; Feng, H.; Zhang, S.; Bu, Q.; Zhang, S.; Qu, J.; Zhang, Y. Super-Eddington Accretion onto the Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124. Astrophys. J. 2019, 873, 19, [arXiv:astro-ph.HE/1901.09485]. https://doi.org/10.3847/1538-435 7/ab0211

2019 arXiv
[118]

Patterns of variability in Be/X-ray pulsars during giant outbursts

Reig, P .; Nespoli, E. Patterns of variability in Be/X-ray pulsars during giant outbursts. Astron. Astrophys. 2013, 551, A1, [arXiv:astro-ph.HE/1212.5944]. https://doi.org/10.1051/0004-6361/201219806

2013 arXiv
[119]

Propeller effect in action in the ultraluminous accreting magnetar M82 X-2

Tsygankov, S.S.; Mushtukov, A.A.; Suleimanov, V .F.; Poutanen, J. Propeller effect in action in the ultraluminous accreting magnetar M82 X-2. Mon. Not. R. Astron. Soc. 2016, 457, 1101–1106, [arXiv:astro-ph.HE/1507.08288]. https://doi.org/10.1093/ mnras/stw046

2016 arXiv
[120]

Propeller Effect in the Transient X-Ray Pulsar SMC X-2

Lutovinov, A.A.; Tsygankov, S.S.; Krivonos, R.A.; Molkov, S.V .; Poutanen, J. Propeller Effect in the Transient X-Ray Pulsar SMC X-2. Astrophys. J. 2017, 834, 209, [arXiv:astro-ph.HE/1607.03427]. https://doi.org/10.3847/1538-4357/834/2/209. Universe 2024, 0, 0 25 of 34

2017 arXiv
[121]

INTEGRAL observations of recurrent fast X-ray transient sources

Sguera, V .; Barlow, E.J.; Bird, A.J.; Clark, D.J.; Dean, A.J.; Hill, A.B.; Moran, L.; Shaw, S.E.; Willis, D.R.; Bazzano, A.; et al. INTEGRAL observations of recurrent fast X-ray transient sources. Astron. Astrophys. 2005, 444, 221–231, [arXiv:astro-ph/astro- ph/0509018]. http...

2005
[122]

Unveiling Supergiant Fast X-Ray Transient Sources with INTEGRAL

Sguera, V .; Bazzano, A.; Bird, A.J.; Dean, A.J.; Ubertini, P .; Barlow, E.J.; Bassani, L.; Clark, D.J.; Hill, A.B.; Malizia, A.; et al. Unveiling Supergiant Fast X-Ray Transient Sources with INTEGRAL. Astrophys. J. 2006, 646, 452–463, [arXiv:astro-ph/astro- ph/0603756]. https...

2006
[123]

The Optical Counterpart to the Peculiar X-Ray Transient XTE J1739-302

Negueruela, I.; Smith, D.M.; Harrison, T.E.; Torrejón, J.M. The Optical Counterpart to the Peculiar X-Ray Transient XTE J1739-302. Astrophys. J. 2006, 638, 982–986, [arXiv:astro-ph/astro-ph/0510675]. https://doi.org/10.1086/498935

2006 arXiv
[124]

Near-infrared Counterparts to Chandra X-ray Sources Toward the Galactic Center

Mauerhan, J.C.; Muno, M.P .; Morris, M.R.; Stolovy, S.R.; Cotera, A. Near-infrared Counterparts to Chandra X-ray Sources Toward the Galactic Center. II. Discovery of Wolf-Rayet Stars and O Supergiants. Astrophys. J. 2010, 710, 706–728, [arXiv:astro- ph.GA/0912.1055]. https://d...

2010 arXiv
[125]

Capturing the lowest luminosity state of the supergiant fast X-ray transient XTE J1739−302

Sidoli, L.; Ponti, G.; Sguera, V .; Esposito, P . Capturing the lowest luminosity state of the supergiant fast X-ray transient XTE J1739−302. Astron. Astrophys. 2023, 671, A150, [arXiv:astro-ph.HE/2301.10533]. https://doi.org/10.1051/0004-6361/202245748

2023 arXiv
[126]

Giant outburst from the supergiant fast X-ray transient IGR J17544-2619: accretion from a transient disc? Astron

Romano, P .; Bozzo, E.; Mangano, V .; Esposito, P .; Israel, G.; Tiengo, A.; Campana, S.; Ducci, L.; Ferrigno, C.; Kennea, J.A. Giant outburst from the supergiant fast X-ray transient IGR J17544-2619: accretion from a transient disc? Astron. Astrophys. 2015, 576, L4, [arXiv:as...

2015 arXiv
[127]

Supergiant Fast X-ray Transients - A short review

Sidoli, L. Supergiant Fast X-ray Transients - A short review. In Proceedings of the XII Multifrequency Behaviour of High Energy Cosmic Sources Workshop (MULTIF2017), 2017, p. 52, [arXiv:astro-ph.HE/1710.03943]. https://doi.org/10.22323/1.306.0052

2017 arXiv
[128]

Monitoring Supergiant Fast X-Ray Transients with Swift

Sidoli, L.; Romano, P .; Mangano, V .; Pellizzoni, A.; Kennea, J.A.; Cusumano, G.; Vercellone, S.; Paizis, A.; Burrows, D.N.; Gehrels, N. Monitoring Supergiant Fast X-Ray Transients with Swift. I. Behavior Outside Outbursts. Astrophys. J. 2008, 687, 1230–1235, [arXiv:astro-ph/...

2008 arXiv
[129]

IGR J16393- 4643: a new heavily-obscured X-ray pulsar

Bodaghee, A.; Walter, R.; Zurita Heras, J.A.; Bird, A.J.; Courvoisier, T.J.L.; Malizia, A.; Terrier, R.; Ubertini, P . IGR J16393- 4643: a new heavily-obscured X-ray pulsar. Astron. Astrophys. 2006, 447, 1027–1034, [arXiv:astro-ph/astro-ph/0510112]. https://doi.org/10.1051/000...

2006 arXiv
[130]

An alternative hypothesis for the outburst mechanism in supergiant fast X-ray transients: the case of IGR J11215-5952

Sidoli, L.; Romano, P .; Mereghetti, S.; Paizis, A.; Vercellone, S.; Mangano, V .; Götz, D. An alternative hypothesis for the outburst mechanism in supergiant fast X-ray transients: the case of IGR J11215-5952. Astron. Astrophys. 2007, 476, 1307–1315, [arXiv:astro-ph/0710.1175...

2007 arXiv
[131]

Discovery of a short orbital period in the Supergiant Fast X-ray Transient IGR J16479-4514

Jain, C.; Paul, B.; Dutta, A. Discovery of a short orbital period in the Supergiant Fast X-ray Transient IGR J16479-4514. Mon. Not. R. Astron. Soc. 2009, 397, L11–L15, [arXiv:astro-ph.HE/0903.5403]. https://doi.org/10.1111/j.1745-3933.2009.00668.x

2009 arXiv
[132]

X-ray pulsations from the region of the supergiant fast X-ray transient IGR J17544-2619

Drave, S.P .; Bird, A.J.; Townsend, L.J.; Hill, A.B.; McBride, V .A.; Sguera, V .; Bazzano, A.; Clark, D.J. X-ray pulsations from the region of the supergiant fast X-ray transient IGR J17544-2619. Astron. Astrophys. 2012, 539, A21, [arXiv:astro-ph.HE/1201.2284]. https://doi.or...

2012 arXiv
[133]

Identification of two new HMXBs in the LMC: an ∼2013 s pulsar and a probable SFXT

Vasilopoulos, G.; Maitra, C.; Haberl, F.; Hatzidimitriou, D.; Petropoulou, M. Identification of two new HMXBs in the LMC: an ∼2013 s pulsar and a probable SFXT. Mon. Not. R. Astron. Soc. 2018, 475, 220–231, [arXiv:astro-ph.HE/1712.00096]. https://doi.org/10.1093/mnras/stx3139

2013 arXiv
[134]

Disentangling the System Geometry of the Supergiant Fast X-Ray Transient IGR J11215-5952 with Swift

Romano, P .; Sidoli, L.; Cusumano, G.; Vercellone, S.; Mangano, V .; Krimm, H.A. Disentangling the System Geometry of the Supergiant Fast X-Ray Transient IGR J11215-5952 with Swift. Astrophys. J. 2009, 696, 2068–2074, [arXiv:astro-ph.HE/0902.1985]. https://doi.org/10.1088/0004...

2009 arXiv
[135]

The 100-month Swift catalogue of supergiant fast X-ray transients

Romano, P .; Evans, P .A.; Bozzo, E.; Mangano, V .; Vercellone, S.; Guidorzi, C.; Ducci, L.; Kennea, J.A.; Barthelmy, S.D.; Palmer, D.M.; et al. The 100-month Swift catalogue of supergiant fast X-ray transients. II. SFXT diagnostics from outburst properties. Astron. Astrophys....

2023 arXiv
[136]

Supergiant Fast X-ray Transients: A New Class of High Mass X-ray Binaries Unveiled by INTEGRAL

Negueruela, I.; Smith, D.M.; Reig, P .; Chaty, S.; Torrejón, J.M. Supergiant Fast X-ray Transients: A New Class of High Mass X-ray Binaries Unveiled by INTEGRAL. In Proceedings of the The X-ray Universe 2005; Wilson, A., Ed., 2006, Vol. 604, ESA Special Publication, p. 165, [a...

2005 doi arXiv
[137]

Expected number of supergiant fast X-ray transients in the Milky Way

Ducci, L.; Doroshenko, V .; Romano, P .; Santangelo, A.; Sasaki, M. Expected number of supergiant fast X-ray transients in the Milky Way. Astron. Astrophys. 2014, 568, A76, [arXiv:astro-ph.HE/1407.5039]. https://doi.org/10.1051/0004-6361/201424215

2014 arXiv
[138]

Be/X-ray binaries as the progenitors of the supergiant fast X-ray transients IGR J18483-0311 and IGR J11215-5952

Liu, Q.Z.; Chaty, S.; Yan, J.Z. Be/X-ray binaries as the progenitors of the supergiant fast X-ray transients IGR J18483-0311 and IGR J11215-5952. Mon. Not. R. Astron. Soc. 2011, 415, 3349–3353. https://doi.org/10.1111/j.1365-2966.2011.18949.x

2011
[139]

Chandra observation of the fast X-ray transient IGR J17544-2619: evidence for a neutron star? Astron

in’t Zand, J.J.M. Chandra observation of the fast X-ray transient IGR J17544-2619: evidence for a neutron star? Astron. Astrophys. 2005, 441, L1–L4, [arXiv:astro-ph/astro-ph/0508240]. https://doi.org/10.1051/0004-6361:200500162

2005 arXiv
[140]

Probing clumpy stellar winds with a neutron star

Walter, R.; Zurita Heras, J. Probing clumpy stellar winds with a neutron star. Astron. Astrophys. 2007, 476, 335–340, [arXiv:astro- ph/0710.2542]. https://doi.org/10.1051/0004-6361:20078353

2007 arXiv
[141]

Measuring the stellar wind parameters in IGR J17544-2619 and Vela X-1 constrains the accretion physics in supergiant fast X-ray transient and classical supergiant X-ray binaries

Giménez-García, A.; Shenar, T.; Torrejón, J.M.; Oskinova, L.; Martínez-Núñez, S.; Hamann, W.R.; Rodes-Roca, J.J.; González-Galán, A.; Alonso-Santiago, J.; González-Fernández, C.; et al. Measuring the stellar wind parameters in IGR J17544-2619 and Vela X-1 constrains the accret...

2016 arXiv
[142]

The stellar and wind parameters of six prototypical HMXBs and their evolutionary status

Hainich, R.; Oskinova, L.M.; Torrejón, J.M.; Fuerst, F.; Bodaghee, A.; Shenar, T.; Sander, A.A.C.; Todt, H.; Spetzer, K.; Hamann, W.R. The stellar and wind parameters of six prototypical HMXBs and their evolutionary status. Astron. Astrophys. 2020, 634, A49, [arXiv:astro-ph.SR...

2020 arXiv
[143]

Bright flares in supergiant fast X-ray transients

Shakura, N.; Postnov, K.; Sidoli, L.; Paizis, A. Bright flares in supergiant fast X-ray transients. Mon. Not. R. Astron. Soc. 2014, 442, 2325–2330, [arXiv:astro-ph.HE/1405.5707]. https://doi.org/10.1093/mnras/stu1027

2014 arXiv
[144]

XMM-Newton and INTEGRAL study of the SFXT IGR J18483-0311 in quiescence: hint of a cyclotron emission feature? Mon

Sguera, V .; Ducci, L.; Sidoli, L.; Bazzano, A.; Bassani, L. XMM-Newton and INTEGRAL study of the SFXT IGR J18483-0311 in quiescence: hint of a cyclotron emission feature? Mon. Not. R. Astron. Soc. 2010, 402, L49–L53, [arXiv:astro-ph.HE/0912.1730]. https://doi.org/10.1111/j.17...

2010 arXiv
[145]

NuSTAR detection of a cyclotron line in the supergiant fast X-ray transient IGR J17544-2619

Bhalerao, V .; Romano, P .; Tomsick, J.; Natalucci, L.; Smith, D.M.; Bellm, E.; Boggs, S.E.; Chakrabarty, D.; Christensen, F.E.; Craig, W.W.; et al. NuSTAR detection of a cyclotron line in the supergiant fast X-ray transient IGR J17544-2619. Mon. Not. R. Astron. Soc. 2015, 447...

2015 arXiv
[146]

NuSTAR and Swift observations of two supergiant fast X-ray transients: AX J1841.0-0536 and SAX J1818.6-1703

Bozzo, E.; Ferrigno, C.; Romano, P . NuSTAR and Swift observations of two supergiant fast X-ray transients: AX J1841.0-0536 and SAX J1818.6-1703. Mon. Not. R. Astron. Soc. 2024, 528, 863–872, [arXiv:astro-ph.HE/2401.03289]. https://doi.org/10.1093/ mnras/stae061

2024 arXiv
[147]

Multi-wavelength observations of IGR J17544-2619 from quiescence to outburst

Bozzo, E.; Bhalerao, V .; Pradhan, P .; Tomsick, J.; Romano, P .; Ferrigno, C.; Chaty, S.; Oskinova, L.; Manousakis, A.; Walter, R.; et al. Multi-wavelength observations of IGR J17544-2619 from quiescence to outburst. Astron. Astrophys. 2016, 596, A16, [arXiv:astro-ph.HE/1610....

2016 arXiv
[148]

Pulse phase-resolved analysis of SMC X-3 during its 2016-2017 super-Eddington outburst

Zhao, H.H.; Weng, S.S.; Ge, M.Y.; Bian, W.H.; Yuan, Q.R. Pulse phase-resolved analysis of SMC X-3 during its 2016-2017 super-Eddington outburst. Astrophys. Space Sci. 2018, 363, 21, [arXiv:astro-ph.HE/1801.02482]. https://doi.org/10.1007/s10509 -017-3245-2

2016 arXiv
[149]

RX J0440.9+4431: another supercritical X-ray pulsar

Salganik, A.; Tsygankov, S.S.; Doroshenko, V .; Molkov, S.V .; Lutovinov, A.A.; Mushtukov, A.A.; Poutanen, J. RX J0440.9+4431: another supercritical X-ray pulsar. Mon. Not. R. Astron. Soc. 2023, 524, 5213–5224, [arXiv:astro-ph.HE/2304.14881]. https: //doi.org/10.1093/mnras/stad2124

2023 arXiv
[150]

Searching for the Highest Energy of Pulsation and Critical Luminosity of Swift J0243.6+6124 Observed by Insight-HXMT

Zhao, Q.X.; Hou, X.; Ge, M.Y.; Zhang, S.N.; Xiao, Y.X.; Tuo, Y.L.; Yang, Z.X.; Kong, L.D.; Qu, J.L.; Zhang, S.; et al. Searching for the Highest Energy of Pulsation and Critical Luminosity of Swift J0243.6+6124 Observed by Insight-HXMT. Research in Astronomy and Astrophysics 2...

2024 arXiv
[151]

Timing Properties of the X-Ray Accreting Pulsar 1A 0535+262 Studied with Insight-HXMT

Wang, P .J.; Kong, L.D.; Zhang, S.; Doroshenko, V .; Santangelo, A.; Ji, L.; Yorgancioglu, E.S.; Chen, Y.P .; Zhang, S.N.; Qu, J.L.; et al. Timing Properties of the X-Ray Accreting Pulsar 1A 0535+262 Studied with Insight-HXMT. Astrophys. J. 2022, 935, 125, [arXiv:astro-ph.HE/2...

2022 arXiv
[152]

Modeling of X-ray pulsars in curved space time

Falkner, S. Modeling of X-ray pulsars in curved space time. PhD thesis, Friedrich Alexander University of Erlangen-Nuremberg, Germany, 2018

2018
[153]

The Transient 42 Second X-Ray Pulsar EXO 2030+375

Parmar, A.N.; White, N.E.; Stella, L. The Transient 42 Second X-Ray Pulsar EXO 2030+375. II. The Luminosity Dependence of the Pulse Profile. Astrophys. J. 1989, 338, 373. https://doi.org/10.1086/167205

1989 doi
[154]

Analyzing X-Ray Pulsar Profiles: Asymmetry as a Key to Geometry and Beam Pattern

Kraus, U.; Nollert, H.P .; Ruder, H.; Riffert, H. Analyzing X-Ray Pulsar Profiles: Asymmetry as a Key to Geometry and Beam Pattern. Astrophys. J. 1995, 450, 763. https://doi.org/10.1086/176182

1995 doi
[155]

Analyzing X-Ray Pulsar Profiles: Geometry and Beam Pattern of Centaurus X-3

Kraus, U.; Blum, S.; Schulte, J.; Ruder, H.; Meszaros, P . Analyzing X-Ray Pulsar Profiles: Geometry and Beam Pattern of Centaurus X-3. Astrophys. J. 1996, 467, 794. https://doi.org/10.1086/177653

1996 doi
[156]

Spectral and Timing Analysis of the Accretion-powered Pulsar 4U 1626-67 Observed with Suzaku and NuSTAR

Iwakiri, W.B.; Pottschmidt, K.; Falkner, S.; Hemphill, P .B.; Fürst, F.; Nishimura, O.; Schwarm, F.W.; Wolff, M.T.; Marcu-Cheatham, D.M.; Chakrabarty, D.; et al. Spectral and Timing Analysis of the Accretion-powered Pulsar 4U 1626-67 Observed with Suzaku and NuSTAR. Astrophys....

2019 arXiv
[157]

Beam Pattern Evolution of Accreting X-Ray Pulsar 1A 0535+262 during Its 2020 Giant Outburst

Hu, Y.F.; Ji, L.; Yu, C.; Wang, P .J.; Doroshenko, V .; Santangelo, A.; Saathoff, I.; Zhang, S.N.; Zhang, S.; Kong, L.D. Beam Pattern Evolution of Accreting X-Ray Pulsar 1A 0535+262 during Its 2020 Giant Outburst. Astrophys. J. 2023, 945, 138, [arXiv:astro- ph.HE/2302.07569]. ...

2020 arXiv
[158]

Blind source separation for decomposing X-ray pulsar profiles

Saathoff, I.; Doroshenko, V .; Santangelo, A. Blind source separation for decomposing X-ray pulsar profiles. Introducing phase-correlated variability analysis (PCVA) with a case study of Cen X-3. Astron. Astrophys. 2024, 683, A52, [arXiv:astro- ph.HE/2401.01226]. https://doi.o...

2024 arXiv
[159]

The giant outburst of EXO 2030+375 I: Spectral and pulse profile evolution

Thalhammer, P .; Ballhausen, R.; Sokolova-Lapa, E.; Stierhof, J.; Zainab, A.; Staubert, R.; Pottschmidt, K.; Coley, J.B.; Rothschild, R.E.; Jaisawal, G.K.; et al. The giant outburst of EXO 2030+375 I: Spectral and pulse profile evolution. arXiv e-prints 2024, p. arXiv:2405.207...

2024 doi arXiv
[160]

Determination of X-ray pulsar geometry with IXPE polarimetry

Doroshenko, V .; Poutanen, J.; Tsygankov, S.S.; Suleimanov, V .F.; Bachetti, M.; Caiazzo, I.; Costa, E.; Di Marco, A.; Heyl, J.; La Monaca, F.; et al. Determination of X-ray pulsar geometry with IXPE polarimetry. Nature Astronomy 2022, 6, 1433–1443, [arXiv:astro-ph.HE/2206.071...

2022 arXiv
[161]

The X-Ray Polarimetry View of the Accreting Pulsar Cen X-3

Tsygankov, S.S.; Doroshenko, V .; Poutanen, J.; Heyl, J.; Mushtukov, A.A.; Caiazzo, I.; Di Marco, A.; Forsblom, S.V .; González- Caniulef, D.; Klawin, M.; et al. The X-Ray Polarimetry View of the Accreting Pulsar Cen X-3. Astrophys. J. Lett. 2022, 941, L14, [arXiv:astro-ph.HE/...

2022 arXiv
[162]

Polarization perspectives on Hercules X-1: further constraining the geometry

Zhao, Q.C.; Li, H.C.; Tao, L.; Feng, H.; Zhang, S.N.; Walter, R.; Ge, M.Y.; Tong, H.; Ji, L.; Zhang, L.; et al. Polarization perspectives on Hercules X-1: further constraining the geometry. Mon. Not. R. Astron. Soc. 2024, 531, 3935–3949, [arXiv:astro- ph.HE/2405.00509]. https:...

2024 arXiv
[163]

Comparing the super-Eddington accretion of SMC X-3 and RX J0209.6-7427 with Swift J0243.6+6124

Liu, J.; Vasilopoulos, G.; Ge, M.; Ji, L.; Weng, S.S.; Zhang, S.N.; Hou, X. Comparing the super-Eddington accretion of SMC X-3 and RX J0209.6-7427 with Swift J0243.6+6124. Mon. Not. R. Astron. Soc. 2022, 517, 3354–3361, [arXiv:astro-ph.HE/2209.11496]. https://doi.org/10.1093/m...

2022 arXiv
[164]

Initial spin periods of neutron stars in supernova remnants

Popov, S.B.; Turolla, R. Initial spin periods of neutron stars in supernova remnants. Astrophys. Space Sci. 2012, 341, 457–464, [arXiv:astro-ph.HE/1204.0632]. https://doi.org/10.1007/s10509-012-1100-z

2012 arXiv
[165]

Initial periods and magnetic fields of neutron stars

Igoshev, A.P .; Frantsuzova, A.; Gourgouliatos, K.N.; Tsichli, S.; Konstantinou, L.; Popov, S.B. Initial periods and magnetic fields of neutron stars. Mon. Not. R. Astron. Soc. 2022, 514, 4606–4619, [arXiv:astro-ph.HE/2205.06823]. https://doi.org/10.1093/ mnras/stac1648

2022 arXiv
[166]

Long-Term Behavior of X-Ray Pulsars in the Small Magellanic Cloud

Laycock, S.; Corbet, R.H.D.; Coe, M.J.; Marshall, F.E.; Markwardt, C.; Lochner, J. Long-Term Behavior of X-Ray Pulsars in the Small Magellanic Cloud. Astrophys. J. Suppl. Ser. 2005, 161, 96–117, [arXiv:astro-ph/astro-ph/0406420]. https://doi.org/10.1086/432884

2005 arXiv
[167]

The First Year of S-CUBED: The Swift Small Magellanic Cloud Survey

Kennea, J.A.; Coe, M.J.; Evans, P .A.; Waters, J.; Jasko, R.E. The First Year of S-CUBED: The Swift Small Magellanic Cloud Survey. Astrophys. J. 2018, 868, 47, [arXiv:astro-ph.HE/1810.05481]. https://doi.org/10.3847/1538-4357/aae839

2018 arXiv
[168]

Spin-up/spin-down of magnetized stars with accretion discs and outflows

Lovelace, R.V .E.; Romanova, M.M.; Bisnovatyi-Kogan, G.S. Spin-up/spin-down of magnetized stars with accretion discs and outflows. Mon. Not. R. Astron. Soc. 1995, 275, 244–254, [arXiv:astro-ph/astro-ph/9412030]. https://doi.org/10.1093/mnras/275. 2.244

1995 arXiv
[169]

Why the Number of Galactic X-ray Stars Is so Small? Astron

Illarionov, A.F.; Sunyaev, R.A. Why the Number of Galactic X-ray Stars Is so Small? Astron. Astrophys. 1975, 39, 185

1975
[170]

Evolution of neutron stars in high-mass X-ray binaries

Urpin, V .; Konenkov, D.; Geppert, U. Evolution of neutron stars in high-mass X-ray binaries. Mon. Not. R. Astron. Soc. 1998, 299, 73–77. https://doi.org/10.1046/j.1365-8711.1998.01771.x

1998
[171]

Evidence for a magnetic neutron star in high-mass X-ray binary 4U 2206+54 with INTEGRAL/IBIS observations

Wang, W. Evidence for a magnetic neutron star in high-mass X-ray binary 4U 2206+54 with INTEGRAL/IBIS observations. Mon. Not. R. Astron. Soc. 2009, 398, 1428–1434, [arXiv:astro-ph.SR/0906.2591]. https://doi.org/10.1111/j.1365-2966.2009.15200.x

2009 arXiv
[172]

Understanding the coexistence of spin-up and spin-down behaviours in long-period X-ray pulsars

Wang, W.; Tong, H. Understanding the coexistence of spin-up and spin-down behaviours in long-period X-ray pulsars. Mon. Not. R. Astron. Soc. 2020, 492, 762–769, [arXiv:astro-ph.HE/1912.03839]. https://doi.org/10.1093/mnras/stz3459

2020 arXiv
[173]

AstroSat and Insight-HXMT Observations of the Long-period X-Ray Pulsar 4U 2206+54.Astrophys

Epili, P .R.; Wang, W. AstroSat and Insight-HXMT Observations of the Long-period X-Ray Pulsar 4U 2206+54.Astrophys. J. 2024, 974, 282, [arXiv:astro-ph.HE/2408.15156]. https://doi.org/10.3847/1538-4357/ad7467

2024 arXiv
[174]

Spin-Down of the Long-Period Accreting Pulsar 4U 2206+54

Finger, M.H.; Ikhsanov, N.R.; Wilson-Hodge, C.A.; Patel, S.K. Spin-Down of the Long-Period Accreting Pulsar 4U 2206+54. Astrophys. J. 2010, 709, 1249–1256, [arXiv:astro-ph.HE/0908.4042]. https://doi.org/10.1088/0004-637X/709/2/1249

2010 arXiv
[175]

Could 2S 0114+650 Be a Magnetar? Astrophys

Li, X.D.; van den Heuvel, E.P .J. Could 2S 0114+650 Be a Magnetar? Astrophys. J. Lett. 1999, 513, L45–L48, [arXiv:astro-ph/astro- ph/9901084]. https://doi.org/10.1086/311904

1999
[176]

Accreting magnetars: a new type of high-mass X-ray binaries?Mon

Reig, P .; Torrejón, J.M.; Blay, P . Accreting magnetars: a new type of high-mass X-ray binaries?Mon. Not. R. Astron. Soc. 2012, 425, 595–604, [arXiv:astro-ph.HE/1203.1490]. https://doi.org/10.1111/j.1365-2966.2012.21509.x

2012 arXiv
[177]

The Broadband Power Spectra of X-Ray Binaries

Wijnands, R.; van der Klis, M. The Broadband Power Spectra of X-Ray Binaries. Astrophys. J. 1999, 514, 939–944, [arXiv:astro- ph/astro-ph/9810342]. https://doi.org/10.1086/306993

1999 arXiv
[178]

Rapid X-ray Variability

van der Klis, M. Rapid X-ray Variability. In Compact stellar X-ray sources; Lewin, W.H.G.; van der Klis, M., Eds.; 2006; Vol. 39, pp. 39–112

2006
[179]

Quasi-periodic Oscillations during a Giant Outburst of A0535+262

Finger, M.H.; Wilson, R.B.; Harmon, B.A. Quasi-periodic Oscillations during a Giant Outburst of A0535+262. Astrophys. J. 1996, 459, 288. https://doi.org/10.1086/176892

1996 doi
[180]

RXTE-PCA observations of 1A 1118-61: timing and spectral studies during an outburst

Devasia, J.; James, M.; Paul, B.; Indulekha, K. RXTE-PCA observations of 1A 1118-61: timing and spectral studies during an outburst. Mon. Not. R. Astron. Soc. 2011, 414, 1023–1031, [arXiv:astro-ph.HE/1101.5020]. https://doi.org/10.1111/j.1365-2966.20 11.18407.x

2011 arXiv
[181]

AstroSat detection of a mHz quasi-periodic oscillation and cyclotron line in IGR J19294+1816 during the 2019 outburst

Raman, G.; Varun.; Paul, B.; Bhattacharya, D. AstroSat detection of a mHz quasi-periodic oscillation and cyclotron line in IGR J19294+1816 during the 2019 outburst. Mon. Not. R. Astron. Soc. 2021, 508, 5578–5586, [arXiv:astro-ph.HE/2109.14022]. https://doi.org/10.1093/mnras/stab2835

2019 arXiv
[182]

Detection of a quasi-periodic oscillation at 40 mHz in Cen X-3 with Insight-HXMT

Liu, Q.; Wang, W.; Chen, X.; Yang, W.; Lu, F.J.; Song, L.M.; Qu, J.L.; Zhang, S.; Zhang, S.N. Detection of a quasi-periodic oscillation at 40 mHz in Cen X-3 with Insight-HXMT. Mon. Not. R. Astron. Soc. 2022, 516, 5579–5587, [arXiv:astro-ph.HE/2209.06662]. https://doi.org/10.10...

2022 arXiv
[183]

Energy dependence of quasi-periodic oscillations in accreting X-ray pulsars

Manikantan, H.; Paul, B.; Sharma, R.; Pradhan, P .; Rana, V . Energy dependence of quasi-periodic oscillations in accreting X-ray pulsars. Mon. Not. R. Astron. Soc. 2024, 531, 530–549, [arXiv:astro-ph.HE/2404.19323]. https://doi.org/10.1093/mnras/stae1170

2024 arXiv
[184]

X-Ray and Optical Observations of A 0535+26

Camero-Arranz, A.; Finger, M.H.; Wilson-Hodge, C.A.; Jenke, P .; Steele, I.; Coe, M.J.; Gutierrez-Soto, J.; Kretschmar, P .; Caballero, I.; Yan, J.; et al. X-Ray and Optical Observations of A 0535+26. Astrophys. J. 2012, 754, 20, [arXiv:astro-ph.HE/1109.3924]. https://doi.org/...

2012 arXiv
[185]

High energy millihertz quasi-periodic oscillations in 1A 0535 + 262 with Insight-HXMT challenge current models

Ma, R.; Tao, L.; Zhang, S.N.; Ji, L.; Zhang, L.; Bu, Q.; Qu, J.; Reig, P .; Méndez, M.; Wang, Y.; et al. High energy millihertz quasi-periodic oscillations in 1A 0535 + 262 with Insight-HXMT challenge current models. Mon. Not. R. Astron. Soc. 2022, 517, 1988–1999, [arXiv:astro...

2022 arXiv
[186]

Is GX5 - 1 a millisecond pulsar? Nature 1985, 316, 239–241

Alpar, M.A.; Shaham, J. Is GX5 - 1 a millisecond pulsar? Nature 1985, 316, 239–241. https://doi.org/10.1038/316239a0

1985 doi
[187]

Intensity and Source State Dependence of the Quasi-periodic Oscillations in Scorpius X-1

van der Klis, M.; Stella, L.; White, N.; Jansen, F.; Parmar, A.N. Intensity and Source State Dependence of the Quasi-periodic Oscillations in Scorpius X-1. Astrophys. J. 1987, 316, 411. https://doi.org/10.1086/165210

1987 doi
[188]

Quasi-Periodic Oscillations in Cen X-3 and the Long-Term Intensity Variations

Raichur, H.; Paul, B. Quasi-Periodic Oscillations in Cen X-3 and the Long-Term Intensity Variations. Astrophys. J. 2008, 685, 1109–1113, [arXiv:astro-ph/0806.0949]. https://doi.org/10.1086/591037

2008 arXiv
[189]

Long-term properties of accretion discs in X-ray binaries - II

Clarkson, W.I.; Charles, P .A.; Coe, M.J.; Laycock, S. Long-term properties of accretion discs in X-ray binaries - II. Stability of radiation-driven warping. Mon. Not. R. Astron. Soc. 2003, 343, 1213–1223, [arXiv:astro-ph/astro-ph/0304073]. https: //doi.org/10.1046/j.1365-8711...

2003 arXiv
[190]

A Systematic Search for Periodicities in RXTE ASM Data

Wen, L.; Levine, A.M.; Corbet, R.H.D.; Bradt, H.V . A Systematic Search for Periodicities in RXTE ASM Data. Astrophys. J. Suppl. Ser. 2006, 163, 372–392, [arXiv:astro-ph/astro-ph/0512529]. https://doi.org/10.1086/500648

2006 arXiv
[191]

Superorbital Periodic Modulation in Wind-accretion High-mass X-Ray Binaries from Swift Burst Alert Telescope Observations

Corbet, R.H.D.; Krimm, H.A. Superorbital Periodic Modulation in Wind-accretion High-mass X-Ray Binaries from Swift Burst Alert Telescope Observations. Astrophys. J. 2013, 778, 45, [arXiv:astro-ph.HE/1309.4119]. https://doi.org/10.1088/0004-637X/77 8/1/45

2013 arXiv
[192]

Precessing warped accretion discs in X-ray binaries

Ogilvie, G.I.; Dubus, G. Precessing warped accretion discs in X-ray binaries. Mon. Not. R. Astron. Soc. 2001, 320, 485–503, [arXiv:astro-ph/astro-ph/0009264]. https://doi.org/10.1046/j.1365-8711.2001.04011.x

2001 arXiv
[193]

Warping and Precession of Accretion Disks around Magnetic Stars: Nonlinear Evolution.Astrophys

Pfeiffer, H.P .; Lai, D. Warping and Precession of Accretion Disks around Magnetic Stars: Nonlinear Evolution.Astrophys. J. 2004, 604, 766–774, [arXiv:astro-ph/astro-ph/0307324]. https://doi.org/10.1086/381967

2004 arXiv
[194]

Characterizing X-ray binary long-term variability

Kotze, M.M.; Charles, P .A. Characterizing X-ray binary long-term variability. Mon. Not. R. Astron. Soc. 2012, 420, 1575–1589, [arXiv:astro-ph.HE/1111.1296]. https://doi.org/10.1111/j.1365-2966.2011.20146.x

2012 arXiv
[195]

EXOSAT Observations of the 35 Day Cycle of Hercules X-1: Evidence for Neutron Star Precession

Truemper, J.; Kahabka, P .; Oegelman, H.; Pietsch, W.; Voges, W. EXOSAT Observations of the 35 Day Cycle of Hercules X-1: Evidence for Neutron Star Precession. Astrophys. J. Lett. 1986, 300, L63. https://doi.org/10.1086/184604

1986 doi
[196]

Variable neutron star free precession in Hercules X-1 from evolution of RXTE X-ray pulse profiles with phase of the 35-d cycle

Postnov, K.; Shakura, N.; Staubert, R.; Kochetkova, A.; Klochkov, D.; Wilms, J. Variable neutron star free precession in Hercules X-1 from evolution of RXTE X-ray pulse profiles with phase of the 35-d cycle. Mon. Not. R. Astron. Soc. 2013, 435, 1147–1164, [arXiv:astro-ph.HE/13...

2013 arXiv
[197]

Very long-term optical variability of high-mass X-ray binaries in the Small Magellanic Cloud

Rajoelimanana, A.F.; Charles, P .A.; Udalski, A. Very long-term optical variability of high-mass X-ray binaries in the Small Magellanic Cloud. Mon. Not. R. Astron. Soc. 2011, 413, 1600–1622, [arXiv:astro-ph.SR/1012.4610]. https://doi.org/10.1111/j.1365 -2966.2011.18243.x

2011 arXiv
[198]

Long-term optical/IR variability of the Be/X-ray binary <ASTROBJ>LS V +44 17</ASTROBJ>/<ASTROBJ>RX J0440.9+4431</ASTROBJ>

Reig, P .; Negueruela, I.; Fabregat, J.; Chato, R.; Coe, M.J. Long-term optical/IR variability of the Be/X-ray binary <ASTROBJ>LS V +44 17</ASTROBJ>/<ASTROBJ>RX J0440.9+4431</ASTROBJ>. Astron. Astrophys. 2005, 440, 1079–1086, [arXiv:astro-ph/astro- ph/0506230]. https://doi.org...

2005
[199]

A Precessing Stellar Disk Model for Superorbital Modulations of the Gamma-Ray Binary LS I+61◦ 303

Chen, A.M.; Takata, J.; Yu, Y.W. A Precessing Stellar Disk Model for Superorbital Modulations of the Gamma-Ray Binary LS I+61◦ 303. Astrophys. J. 2024, 973, 162. https://doi.org/10.3847/1538-4357/ad6b0a

2024 doi
[200]

Study of the accreting pulsar 4U 0115+63 using a bulk and thermal Comptonization model

Ferrigno, C.; Becker, P .A.; Segreto, A.; Mineo, T.; Santangelo, A. Study of the accreting pulsar 4U 0115+63 using a bulk and thermal Comptonization model. Astron. Astrophys. 2009, 498, 825–836, [arXiv:astro-ph.HE/0902.4392]. https://doi.org/10.1051/ 0004-6361/200809373

2009 arXiv
[201]

A Reflection Model for the Cyclotron Lines in the Spectra of X-Ray Pulsars

Poutanen, J.; Mushtukov, A.A.; Suleimanov, V .F.; Tsygankov, S.S.; Nagirner, D.I.; Doroshenko, V .; Lutovinov, A.A. A Reflection Model for the Cyclotron Lines in the Spectra of X-Ray Pulsars. Astrophys. J. 2013, 777, 115, [arXiv:astro-ph.HE/1304.2633]. https://doi.org/10.1088/...

2013 arXiv
[202]

Cyclotron line formation by reflection on the surface of a magnetic neutron star

Kylafis, N.D.; Trümper, J.E.; Loudas, N.A. Cyclotron line formation by reflection on the surface of a magnetic neutron star. Astron. Astrophys. 2021, 655, A39, [arXiv:astro-ph.HE/2108.07573]. https://doi.org/10.1051/0004-6361/202039361

2021 arXiv
[203]

Cyclotron line variability

Mihara, T.; Makishima, K.; Nagase, F. Cyclotron line variability. Advances in Space Research 1998, 22, 987–996, [arXiv:astro- ph.HE/1401.5138]. https://doi.org/10.1016/S0273-1177(98)00128-8

1998 arXiv
[204]

Magnetic Fields of Accreting X-Ray Pulsars with the Rossi X-Ray Timing Explorer

Coburn, W.; Heindl, W.A.; Rothschild, R.E.; Gruber, D.E.; Kreykenbohm, I.; Wilms, J.; Kretschmar, P .; Staubert, R. Magnetic Fields of Accreting X-Ray Pulsars with the Rossi X-Ray Timing Explorer. Astrophys. J. 2002, 580, 394–412, [arXiv:astro-ph/astro- ph/0207325]. https://do...

2002
[205]

NuSTAR and XMM-Newton observations of SXP 59 during its 2017 giant outburst

Weng, S.S.; Ge, M.Y.; Zhao, H.H. NuSTAR and XMM-Newton observations of SXP 59 during its 2017 giant outburst. Mon. Not. R. Astron. Soc. 2019, 489, 1000–1005, [arXiv:astro-ph.HE/1908.04908]. https://doi.org/10.1093/mnras/stz2267

2017 arXiv
[206]

Generalized Comptonization Models and Application to the Recent High-Energy Observations

Titarchuk, L. Generalized Comptonization Models and Application to the Recent High-Energy Observations. Astrophys. J. 1994, 434, 570. https://doi.org/10.1086/174760

1994 doi
[207]

A New Comptonization Model for Weakly Magnetized, Accreting Neutron Stars in Low-Mass X-Ray Binaries

Farinelli, R.; Titarchuk, L.; Paizis, A.; Frontera, F. A New Comptonization Model for Weakly Magnetized, Accreting Neutron Stars in Low-Mass X-Ray Binaries. Astrophys. J. 2008, 680, 602–614, [arXiv:astro-ph/0802.2639]. https://doi.org/10.1086/587162

2008 arXiv
[208]

Numerical solution of the radiative transfer equation: X-ray spectral forma- tion from cylindrical accretion onto a magnetized neutron star

Farinelli, R.; Ceccobello, C.; Romano, P .; Titarchuk, L. Numerical solution of the radiative transfer equation: X-ray spectral forma- tion from cylindrical accretion onto a magnetized neutron star. Astron. Astrophys. 2012, 538, A67, [arXiv:astro-ph.HE/1111.6851]. https://doi....

2012 arXiv
[209]

The NuSTAR X-Ray Spectrum of Hercules X-1: A Radiation-dominated Radiative Shock.Astrophys

Wolff, M.T.; Becker, P .A.; Gottlieb, A.M.; Fürst, F.; Hemphill, P .B.; Marcu-Cheatham, D.M.; Pottschmidt, K.; Schwarm, F.W.; Wilms, J.; Wood, K.S. The NuSTAR X-Ray Spectrum of Hercules X-1: A Radiation-dominated Radiative Shock.Astrophys. J. 2016, 831, 194, [arXiv:astro-ph.HE...

2016 arXiv
[210]

RX J0440.9 + 4431: a persistent Be/X-ray binary in outburst

Ferrigno, C.; Farinelli, R.; Bozzo, E.; Pottschmidt, K.; Klochkov, D.; Kretschmar, P . RX J0440.9 + 4431: a persistent Be/X-ray binary in outburst. Astron. Astrophys. 2013, 553, A103, [arXiv:astro-ph.HE/1303.7087]. https://doi.org/10.1051/0004-6361/201321053

2013 arXiv
[211]

A new model for the X-ray continuum of the magnetized accreting pulsars

Farinelli, R.; Ferrigno, C.; Bozzo, E.; Becker, P .A. A new model for the X-ray continuum of the magnetized accreting pulsars. Astron. Astrophys. 2016, 591, A29, [arXiv:astro-ph.HE/1602.04308]. https://doi.org/10.1051/0004-6361/201527257

2016 arXiv
[212]

Fitting strategies of accretion column models and application to the broadband spectrum of Cen X-3

Thalhammer, P .; Bissinger, M.; Ballhausen, R.; Pottschmidt, K.; Wolff, M.T.; Stierhof, J.; Sokolova-Lapa, E.; Fürst, F.; Malacaria, C.; Gottlieb, A.; et al. Fitting strategies of accretion column models and application to the broadband spectrum of Cen X-3. Astron. Astrophys. ...

2021 arXiv
[213]

A Comprehensive Comparison of Spin-up and Spin-down Episodes of 4U 1538-522 Observed with NuSTAR

Hu, Y.; Ji, L.; Yu, C.; Yang, L. A Comprehensive Comparison of Spin-up and Spin-down Episodes of 4U 1538-522 Observed with NuSTAR. Astrophys. J. 2024, 971, 120, [arXiv:astro-ph.HE/2406.12155]. https://doi.org/10.3847/1538-4357/ad58d2. Universe 2024, 0, 0 29 of 34

2024 arXiv
[214]

Rapid spectral and timing variability of Be/X-ray binaries during type ;II outbursts.Astron

Reig, P . Rapid spectral and timing variability of Be/X-ray binaries during type ;II outbursts.Astron. Astrophys. 2008, 489, 725–740, [arXiv:astro-ph/0807.4786]. https://doi.org/10.1051/0004-6361:200810021

2008 arXiv
[215]

Luminosity dependence of the cyclotron line and evidence for the accretion regime transition in V 0332+53

Doroshenko, V .; Tsygankov, S.S.; Mushtukov, A.A.; Lutovinov, A.A.; Santangelo, A.; Suleimanov, V .F.; Poutanen, J. Luminosity dependence of the cyclotron line and evidence for the accretion regime transition in V 0332+53. Mon. Not. R. Astron. Soc. 2017, 466, 2143–2150, [arXiv...

2017 arXiv
[216]

NICER and Fermi GBM Observations of the First Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124

Wilson-Hodge, C.A.; Malacaria, C.; Jenke, P .A.; Jaisawal, G.K.; Kerr, M.; Wolff, M.T.; Arzoumanian, Z.; Chakrabarty, D.; Doty, J.P .; Gendreau, K.C.; et al. NICER and Fermi GBM Observations of the First Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124. Astrophys. J. 201...

2018 arXiv
[217]

Insight-HXMT observations of Swift J0243.6+6124: the evolution of RMS pulse fractions at super-Eddington luminosity

Wang, P .J.; Kong, L.D.; Zhang, S.; Chen, Y.P .; Zhang, S.N.; Qu, J.L.; Ji, L.; Tao, L.; Ge, M.Y.; Lu, F.J.; et al. Insight-HXMT observations of Swift J0243.6+6124: the evolution of RMS pulse fractions at super-Eddington luminosity. Mon. Not. R. Astron. Soc. 2020, 497, 5498–55...

2020
[218]

Luminosity Dependence of the Cyclotron Line Energy in 1A 0535+262 Observed by Insight-HXMT during the 2020 Giant Outburst

Kong, L.D.; Zhang, S.; Ji, L.; Reig, P .; Doroshenko, V .; Santangelo, A.; Staubert, R.; Zhang, S.N.; Soria, R.; Chang, Z.; et al. Luminosity Dependence of the Cyclotron Line Energy in 1A 0535+262 Observed by Insight-HXMT during the 2020 Giant Outburst. Astrophys. J. Lett. 202...

2020 arXiv
[219]

Cyclotron emission, absorption, and the two faces of X-ray pulsar A 0535+262

Tsygankov, S.S.; Doroshenko, V .; Mushtukov, A.A.; Suleimanov, V .F.; Lutovinov, A.A.; Poutanen, J. Cyclotron emission, absorption, and the two faces of X-ray pulsar A 0535+262. Mon. Not. R. Astron. Soc. 2019, 487, L30–L34, [arXiv:astro- ph.HE/1905.09496]. https://doi.org/10.1...

2019 arXiv
[220]

Dramatic spectral transition of X-ray pulsar GX 304-1 in low luminous state

Tsygankov, S.S.; Rouco Escorial, A.; Suleimanov, V .F.; Mushtukov, A.A.; Doroshenko, V .; Lutovinov, A.A.; Wijnands, R.; Poutanen, J. Dramatic spectral transition of X-ray pulsar GX 304-1 in low luminous state. Mon. Not. R. Astron. Soc. 2019, 483, L144–L148, [arXiv:astro-ph.HE...

2019 arXiv
[221]

The hard X-ray emission of X Persei

Doroshenko, V .; Santangelo, A.; Kreykenbohm, I.; Doroshenko, R. The hard X-ray emission of X Persei. Astron. Astrophys. 2012, 540, L1, [arXiv:astro-ph.HE/1202.6271]. https://doi.org/10.1051/0004-6361/201218878

2012 arXiv
[222]

A Transition Discovered in the Subcritical Regime of 1A 0535+262

Xiao, H.; Ji, L. A Transition Discovered in the Subcritical Regime of 1A 0535+262. Astrophys. J. 2024, 963, 42, [arXiv:astro- ph.HE/2401.15429]. https://doi.org/10.3847/1538-4357/ad23cd

2024 arXiv
[223]

Origin of the Soft Excess in X-Ray Pulsars

Hickox, R.C.; Narayan, R.; Kallman, T.R. Origin of the Soft Excess in X-Ray Pulsars. Astrophys. J. 2004, 614, 881–896, [arXiv:astro- ph/astro-ph/0407115]. https://doi.org/10.1086/423928

2004 arXiv
[224]

An investigation of the ’10 keV feature’ in the spectra of accretion powered X-ray pulsars with NuSTAR

Manikantan, H.; Paul, B.; Rana, V . An investigation of the ’10 keV feature’ in the spectra of accretion powered X-ray pulsars with NuSTAR. Mon. Not. R. Astron. Soc. 2023, 526, 1–28, [arXiv:astro-ph.HE/2308.15129]. https://doi.org/10.1093/mnras/stad2527

2023 arXiv
[225]

On the Absorption of X-Rays in the Interstellar Medium

Wilms, J.; Allen, A.; McCray, R. On the Absorption of X-Rays in the Interstellar Medium. Astrophys. J. 2000, 542, 914–924, [arXiv:astro-ph/astro-ph/0008425]. https://doi.org/10.1086/317016

2000 arXiv
[226]

Pulse Phase-Resolved Analysis of the High-Mass X-Ray Binary Centaurus X-3 over Two Binary Orbits.Astrophys

Suchy, S.; Pottschmidt, K.; Wilms, J.; Kreykenbohm, I.; Schönherr, G.; Kretschmar, P .; McBride, V .; Caballero, I.; Rothschild, R.E.; Grinberg, V . Pulse Phase-Resolved Analysis of the High-Mass X-Ray Binary Centaurus X-3 over Two Binary Orbits.Astrophys. J. 2008, 675, 1487–1...

2008 arXiv
[227]

Orbital phase resolved spectroscopy of GX 301-2 with MAXI

Islam, N.; Paul, B. Orbital phase resolved spectroscopy of GX 301-2 with MAXI. Mon. Not. R. Astron. Soc. 2014, 441, 2539–2545, [arXiv:astro-ph.HE/1404.3902]. https://doi.org/10.1093/mnras/stu756

2014 arXiv
[228]

Studying the X-ray absorption characteristics of Centaurus X-3 using nearly 14 years of MAXI/GSC data

Balu, A.; Roy, K.; Manikantan, H.; Tamang, A.; Paul, B. Studying the X-ray absorption characteristics of Centaurus X-3 using nearly 14 years of MAXI/GSC data. arXiv e-prints 2024, p. arXiv:2410.17695, [arXiv:astro-ph.HE/2410.17695]. https: //doi.org/10.48550/arXiv.2410.17695

2024 doi arXiv
[229]

Chandra Grating Spectroscopy of the Be/X-ray Binary 1A 0535+262.Astrophys

Reynolds, M.T.; Miller, J.M. Chandra Grating Spectroscopy of the Be/X-ray Binary 1A 0535+262.Astrophys. J. 2010, 723, 1799–1805, [arXiv:astro-ph.HE/1009.2240]. https://doi.org/10.1088/0004-637X/723/2/1799

2010 arXiv
[230]

A Fast X-ray Disk Wind in the Transient Pulsar IGR J17480-2446 in Terzan 5

Miller, J.M.; Maitra, D.; Cackett, E.M.; Bhattacharyya, S.; Strohmayer, T.E. A Fast X-ray Disk Wind in the Transient Pulsar IGR J17480-2446 in Terzan 5. Astrophys. J. Lett. 2011, 731, L7, [arXiv:astro-ph.HE/1101.2377]. https://doi.org/10.1088/2041-8205/73 1/1/L7

2011 arXiv
[231]

An ionized accretion disc wind in Hercules X-1.Mon

Kosec, P .; Fabian, A.C.; Pinto, C.; Walton, D.J.; Dyda, S.; Reynolds, C.S. An ionized accretion disc wind in Hercules X-1.Mon. Not. R. Astron. Soc. 2020, 491, 3730–3750, [arXiv:astro-ph.HE/1910.08337]. https://doi.org/10.1093/mnras/stz3200

2020 arXiv
[233]

Vertical wind structure in an X-ray binary revealed by a precessing accretion disk

Kosec, P .; Kara, E.; Fabian, A.C.; Fürst, F.; Pinto, C.; Psaradaki, I.; Reynolds, C.S.; Rogantini, D.; Walton, D.J.; Ballhausen, R.; et al. Vertical wind structure in an X-ray binary revealed by a precessing accretion disk. Nature Astronomy 2023, 7, 715–723, [arXiv:astro-ph.H...

2023 arXiv
[234]

A Chandra Survey of Fluorescence Fe Lines in X-ray Binaries at High Resolution

Torrejón, J.M.; Schulz, N.S.; Nowak, M.A.; Kallman, T.R. A Chandra Survey of Fluorescence Fe Lines in X-ray Binaries at High Resolution. Astrophys. J. 2010, 715, 947–958, [arXiv:astro-ph.HE/1004.2345]. https://doi.org/10.1088/0004-637X/715/2/947

2010 arXiv
[235]

New Constraints on the Geometry and Kinematics of Matter Surrounding the Accretion Flow in X-Ray Binaries from Chandra High-energy Transmission Grating X-Ray Spectroscopy

Tzanavaris, P .; Yaqoob, T. New Constraints on the Geometry and Kinematics of Matter Surrounding the Accretion Flow in X-Ray Binaries from Chandra High-energy Transmission Grating X-Ray Spectroscopy. Astrophys. J. 2018, 855, 25, [arXiv:astro- ph.HE/1801.08544]. https://doi.org...

2018 arXiv
[236]

X-Ray Reprocessing: Through the Eclipse Spectra of High-mass X-Ray Binaries with XMM- Newton

Aftab, N.; Paul, B.; Kretschmar, P . X-Ray Reprocessing: Through the Eclipse Spectra of High-mass X-Ray Binaries with XMM- Newton. Astrophys. J. Suppl. Ser. 2019, 243, 29, [arXiv:astro-ph.HE/1906.07739]. https://doi.org/10.3847/1538-4365/ab2a77. Universe 2024, 0, 0 30 of 34

2019 arXiv
[237]

X-ray reprocessing in accreting pulsar GX 301-2 observed with Insight-HXMT

Ji, L.; Doroshenko, V .; Suleimanov, V .; Santangelo, A.; Orlandini, M.; Liu, J.; Ducci, L.; Zhang, S.N.; Nabizadeh, A.; Gavran, D.; et al. X-ray reprocessing in accreting pulsar GX 301-2 observed with Insight-HXMT. Mon. Not. R. Astron. Soc. 2021, 501, 2522–2530, [arXiv:astro-...

2021 arXiv
[238]

Evidence for strong cyclotron line emission in the hard X-ray spectrum of Hercules X-1

Truemper, J.; Pietsch, W.; Reppin, C.; Voges, W.; Staubert, R.; Kendziorra, E. Evidence for strong cyclotron line emission in the hard X-ray spectrum of Hercules X-1. Astrophys. J. Lett. 1978, 219, L105–L110. https://doi.org/10.1086/182617

1978 doi
[239]

Discovery of a Third Harmonic Cyclotron Resonance Scattering Feature in the X-Ray Spectrum of 4U 0115+63

Heindl, W.A.; Coburn, W.; Gruber, D.E.; Pelling, M.R.; Rothschild, R.E.; Wilms, J.; Pottschmidt, K.; Staubert, R. Discovery of a Third Harmonic Cyclotron Resonance Scattering Feature in the X-Ray Spectrum of 4U 0115+63. Astrophys. J. Lett. 1999, 521, L49–L53, [arXiv:astro-ph/a...

1999 arXiv
[240]

A BEPPOSAX Study of the Pulsating Transient X0115+63: The First X-Ray Spectrum with Four Cyclotron Harmonic Features

Santangelo, A.; Segreto, A.; Giarrusso, S.; Dal Fiume, D.; Orlandini, M.; Parmar, A.N.; Oosterbroek, T.; Bulik, T.; Mihara, T.; Campana, S.; et al. A BEPPOSAX Study of the Pulsating Transient X0115+63: The First X-Ray Spectrum with Four Cyclotron Harmonic Features. Astrophys. ...

1999 doi
[241]

A tale of two periods: determination of the orbital ephemeris of the super-Eddington pulsar NGC 7793 P13

Fürst, F.; Walton, D.J.; Heida, M.; Harrison, F.A.; Barret, D.; Brightman, M.; Fabian, A.C.; Middleton, M.J.; Pinto, C.; Rana, V .; et al. A tale of two periods: determination of the orbital ephemeris of the super-Eddington pulsar NGC 7793 P13. Astron. Astrophys. 2018, 616, A1...

2018 arXiv
[242]

A Peculiar Cyclotron Line near 16 keV Detected in the 2015 Outburst of 4U 0115+63? Astrophys

Liu, B.S.; Tao, L.; Zhang, S.N.; Li, X.D.; Ge, M.Y.; Qu, J.L.; Song, L.M.; Ji, L.; Zhang, S.; Santangelo, A.; et al. A Peculiar Cyclotron Line near 16 keV Detected in the 2015 Outburst of 4U 0115+63? Astrophys. J. 2020, 900, 41, [arXiv:astro-ph.HE/1911.12025]. https://doi.org/...

2015 arXiv
[243]

Luminosity dependence of the multiple cyclotron lines in 4U 0115+63

Roy, K.; Manikantan, H.; Paul, B. Luminosity dependence of the multiple cyclotron lines in 4U 0115+63. Astron. Astrophys. 2024, 690, A50, [arXiv:astro-ph.HE/2407.13869]. https://doi.org/10.1051/0004-6361/202450395

2024 arXiv
[244]

An in-depth analysis of the variable cyclotron lines in GX 301 −2

Zalot, N.; Sokolova-Lapa, E.; Stierhof, J.; Ballhausen, R.; Zainab, A.; Pottschmidt, K.; Fürst, F.; Thalhammer, P .; Islam, N.; Diez, C.M.; et al. An in-depth analysis of the variable cyclotron lines in GX 301 −2. Astron. Astrophys. 2024, 686, A95, [arXiv:astro-ph.HE/2403.1168...

2024 arXiv
[245]

X-ray pulsar models

Meszaros, P .; Nagel, W. X-ray pulsar models. I. Angle-dependent cyclotron line formation and comptonization.Astrophys. J. 1985, 298, 147–160. https://doi.org/10.1086/163594

1985 doi
[246]

Formation Mechanism for Broad and Shallow Profiles of Cyclotron Lines in Accreting X-Ray Pulsars

Nishimura, O. Formation Mechanism for Broad and Shallow Profiles of Cyclotron Lines in Accreting X-Ray Pulsars. Astrophys. J. 2008, 672, 1127–1136. https://doi.org/10.1086/523782

2008 doi
[247]

Superposition of Cyclotron Lines in Accreting X-Ray Pulsars

Nishimura, O. Superposition of Cyclotron Lines in Accreting X-Ray Pulsars. I. Long Spin Period. Astrophys. J. 2011, 730, 106. https://doi.org/10.1088/0004-637X/730/2/106

2011 doi
[248]

Variations of Cyclotron Line Energy with Luminosity in Accreting X-Ray Pulsars

Nishimura, O. Variations of Cyclotron Line Energy with Luminosity in Accreting X-Ray Pulsars. Astrophys. J. 2014, 781, 30. https://doi.org/10.1088/0004-637X/781/1/30

2014 doi
[249]

Influence of bulk motion of an infalling plasma in line-forming region on cyclotron line in accreting X-ray pulsars

Nishimura, O. Influence of bulk motion of an infalling plasma in line-forming region on cyclotron line in accreting X-ray pulsars. Publ. Astron. Soc. Pac. 2019, 71, 42. https://doi.org/10.1093/pasj/psz008

2019 doi
[250]

Variations in energy of cyclotron lines with double structures formed in a line-forming region with bulk motion in accreting X-ray pulsars

Nishimura, O. Variations in energy of cyclotron lines with double structures formed in a line-forming region with bulk motion in accreting X-ray pulsars. Publ. Astron. Soc. Pac. 2022, 74, 961–973. https://doi.org/10.1093/pasj/psac048

2022 doi
[251]

Cyclotron resonant scattering feature simulations

Schwarm, F.W.; Schönherr, G.; Falkner, S.; Pottschmidt, K.; Wolff, M.T.; Becker, P .A.; Sokolova-Lapa, E.; Klochkov, D.; Ferrigno, C.; Fürst, F.; et al. Cyclotron resonant scattering feature simulations. I. Thermally averaged cyclotron scattering cross sections, mean free phot...

2017 arXiv
[252]

Cyclotron resonant scattering feature simulations

Schwarm, F.W.; Ballhausen, R.; Falkner, S.; Schönherr, G.; Pottschmidt, K.; Wolff, M.T.; Becker, P .A.; Fürst, F.; Marcu-Cheatham, D.M.; Hemphill, P .B.; et al. Cyclotron resonant scattering feature simulations. II. Description of the CRSF simulation process. Astron. Astrophys...

2017 arXiv
[253]

A new Monte Carlo radiative transfer simulation of cyclotron resonant scattering features

Kumar, S.; Bala, S.; Bhattacharya, D. A new Monte Carlo radiative transfer simulation of cyclotron resonant scattering features. Mon. Not. R. Astron. Soc. 2022, 515, 914–927, [arXiv:astro-ph.HE/2207.00657]. https://doi.org/10.1093/mnras/stac1871

2022 arXiv
[254]

Cyclotron line formation in the radiative shock of an accreting magnetized neutron star

Loudas, N.; Kylafis, N.D.; Trümper, J. Cyclotron line formation in the radiative shock of an accreting magnetized neutron star. Astron. Astrophys. 2024, 685, A95, [arXiv:astro-ph.HE/2402.07983]. https://doi.org/10.1051/0004-6361/202348109

2024 arXiv
[255]

A phase-dependent view of cyclotron lines from model accretion mounds on neutron stars

Mukherjee, D.; Bhattacharya, D. A phase-dependent view of cyclotron lines from model accretion mounds on neutron stars. Mon. Not. R. Astron. Soc. 2012, 420, 720–731, [arXiv:astro-ph.HE/1110.2850]. https://doi.org/10.1111/j.1365-2966.2011.20085.x

2012 arXiv
[256]

Insight- HXMT Discovery of the Highest-energy CRSF from the First Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124

Kong, L.D.; Zhang, S.; Zhang, S.N.; Ji, L.; Doroshenko, V .; Santangelo, A.; Chen, Y.P .; Lu, F.J.; Ge, M.Y.; Wang, P .J.; et al. Insight- HXMT Discovery of the Highest-energy CRSF from the First Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124. Astrophys. J. Lett. 2022,...

2022 arXiv
[257]

Discovery of a flux-related change of the cyclotron line energy in Hercules X-1

Staubert, R.; Shakura, N.I.; Postnov, K.; Wilms, J.; Rothschild, R.E.; Coburn, W.; Rodina, L.; Klochkov, D. Discovery of a flux-related change of the cyclotron line energy in Hercules X-1. Astron. Astrophys. 2007, 465, L25–L28, [arXiv:astro-ph/astro-ph/0702490]. https://doi.or...

2007 arXiv
[258]

Discovery and modelling of a flattening of the positive cyclotron line/luminosity relation in GX 304-1 with RXTE

Rothschild, R.E.; Kühnel, M.; Pottschmidt, K.; Hemphill, P .; Postnov, K.; Gornostaev, M.; Shakura, N.; Fürst, F.; Wilms, J.; Staubert, R.; et al. Discovery and modelling of a flattening of the positive cyclotron line/luminosity relation in GX 304-1 with RXTE. Mon. Not. R. Ast...

2017 arXiv
[259]

Positive correlation between the cyclotron line energy and luminosity in sub-critical X-ray pulsars: Doppler effect in the accretion channel

Mushtukov, A.A.; Tsygankov, S.S.; Serber, A.V .; Suleimanov, V .F.; Poutanen, J. Positive correlation between the cyclotron line energy and luminosity in sub-critical X-ray pulsars: Doppler effect in the accretion channel. Mon. Not. R. Astron. Soc. 2015, 454, 2714–2721, [arXiv...

2015 arXiv
[260]

Changes in the cyclotron line energy on short and long timescales in V 0332+53

Vybornov, V .; Doroshenko, V .; Staubert, R.; Santangelo, A. Changes in the cyclotron line energy on short and long timescales in V 0332+53. Astron. Astrophys. 2018, 610, A88, [arXiv:astro-ph.HE/1801.01349]. https://doi.org/10.1051/0004-6361/201731750

2018 arXiv
[261]

Cyclotron line evolution revealed with pulse-to-pulse analysis in the 2020 outburst of 1A 0535+262

Shui, Q.C.; Zhang, S.; Wang, P .J.; Mushtukov, A.A.; Santangelo, A.; Zhang, S.N.; Kong, L.D.; Ji, L.; Chen, Y.P .; Doroshenko, V .; et al. Cyclotron line evolution revealed with pulse-to-pulse analysis in the 2020 outburst of 1A 0535+262. Mon. Not. R. Astron. Soc. 2024, 528, 7...

2020 arXiv
[262]

A quantitative explanation of the cyclotron-line variation in accreting magnetic neutron stars of super-critical luminosity

Loudas, N.; Kylafis, N.D.; Trümper, J. A quantitative explanation of the cyclotron-line variation in accreting magnetic neutron stars of super-critical luminosity. Astron. Astrophys. 2024, 689, A75, [arXiv:astro-ph.HE/2406.09511]. https://doi.org/10.1051/00 04-6361/202449695

2024 arXiv
[263]

Long-term change in the cyclotron line energy in Hercules X-1

Staubert, R.; Klochkov, D.; Wilms, J.; Postnov, K.; Shakura, N.I.; Rothschild, R.E.; Fürst, F.; Harrison, F.A. Long-term change in the cyclotron line energy in Hercules X-1. Astron. Astrophys. 2014, 572, A119, [arXiv:astro-ph.HE/1410.3647]. https: //doi.org/10.1051/0004-6361/201424203

2014 arXiv
[264]

Continued decay in the cyclotron line energy in Hercules X-1

Staubert, R.; Klochkov, D.; Vybornov, V .; Wilms, J.; Harrison, F.A. Continued decay in the cyclotron line energy in Hercules X-1. Astron. Astrophys. 2016, 590, A91, [arXiv:astro-ph.HE/1603.07090]. https://doi.org/10.1051/0004-6361/201527955

2016 arXiv
[265]

Cyclotron line energy in Hercules X-1: stable after the decay

Staubert, R.; Ducci, L.; Ji, L.; Fürst, F.; Wilms, J.; Rothschild, R.E.; Pottschmidt, K.; Brumback, M.; Harrison, F. Cyclotron line energy in Hercules X-1: stable after the decay. Astron. Astrophys. 2020, 642, A196, [arXiv:astro-ph.HE/2008.13434]. https://doi.org/10.1051/0004-...

2020 arXiv
[266]

Constant cyclotron line energy in Hercules X-1 - Joint Insight-HXMT and NuSTAR observations

Xiao, G.C.; Ji, L.; Staubert, R.; Ge, M.Y.; Zhang, S.; Zhang, S.N.; Santangelo, A.; Ducci, L.; Liao, J.Y.; Guo, C.C.; et al. Constant cyclotron line energy in Hercules X-1 - Joint Insight-HXMT and NuSTAR observations. Journal of High Energy Astrophysics 2019, 23, 29–32, [arXiv...

2019
[267]

Swift/BAT measurements of the cyclotron line energy decay in the accreting neutron star Hercules X-1: indication of an evolution of the magnetic field? Astron

Klochkov, D.; Staubert, R.; Postnov, K.; Wilms, J.; Rothschild, R.E.; Santangelo, A. Swift/BAT measurements of the cyclotron line energy decay in the accreting neutron star Hercules X-1: indication of an evolution of the magnetic field? Astron. Astrophys. 2015, 578, A88, [arXi...

2015 arXiv
[268]

The Swift-BAT monitoring reveals a long-term decay of the cyclotron line energy in Vela X-1

La Parola, V .; Cusumano, G.; Segreto, A.; D’Aì, A. The Swift-BAT monitoring reveals a long-term decay of the cyclotron line energy in Vela X-1. Mon. Not. R. Astron. Soc. 2016, 463, 185–190, [arXiv:astro-ph.HE/1608.06429]. https://doi.org/10.1093/ mnras/stw1915

2016 arXiv
[269]

Long-term evolutions of the cyclotron line energies in Her X-1, Vela X-1, and Cen X-3 as observed with Swift/BAT.Mon

Ji, L.; Staubert, R.; Ducci, L.; Santangelo, A.; Zhang, S.; Chang, Z. Long-term evolutions of the cyclotron line energies in Her X-1, Vela X-1, and Cen X-3 as observed with Swift/BAT.Mon. Not. R. Astron. Soc. 2019, 484, 3797–3805, [arXiv:astro-ph.HE/1901.07269]. https://doi.or...

2019 arXiv
[270]

Radiative transfer in a strongly magnetized plasma

Nagel, W. Radiative transfer in a strongly magnetized plasma. I - Effects of anisotropy. II - Effects of Comptonization. Astrophys. J. 1981, 251, 278–296. https://doi.org/10.1086/159463

1981 doi
[271]

Polarization of accreting X-ray pulsars - II

Caiazzo, I.; Heyl, J. Polarization of accreting X-ray pulsars - II. Hercules X-1. Mon. Not. R. Astron. Soc. 2021, 501, 129–136, [arXiv:astro-ph.HE/2009.00634]. https://doi.org/10.1093/mnras/staa3429

2021 arXiv
[272]

X-ray pulsar GRO J1008 −57 as an orthogonal rotator

Tsygankov, S.S.; Doroshenko, V .; Mushtukov, A.A.; Poutanen, J.; Di Marco, A.; Heyl, J.; La Monaca, F.; Forsblom, S.V .; Malacaria, C.; Marshall, H.L.; et al. X-ray pulsar GRO J1008 −57 as an orthogonal rotator. Astron. Astrophys. 2023, 675, A48, [arXiv:astro- ph.HE/2302.06680...

2023 arXiv
[273]

X-ray polarimetry of X-ray pulsar X Persei: another orthogonal rotator? Mon

Mushtukov, A.A.; Tsygankov, S.S.; Poutanen, J.; Doroshenko, V .; Salganik, A.; Costa, E.; Marco, A.D.; Heyl, J.; Monaca, F.L.; Lutovinov, A.A.; et al. X-ray polarimetry of X-ray pulsar X Persei: another orthogonal rotator? Mon. Not. R. Astron. Soc. 2023, 524, 2004–2014, [arXiv...

2023 arXiv
[274]

IXPE Observations of the Quintessential Wind-accreting X-Ray Pulsar Vela X-1

Forsblom, S.V .; Poutanen, J.; Tsygankov, S.S.; Bachetti, M.; Di Marco, A.; Doroshenko, V .; Heyl, J.; La Monaca, F.; Malacaria, C.; Marshall, H.L.; et al. IXPE Observations of the Quintessential Wind-accreting X-Ray Pulsar Vela X-1. Astrophys. J. Lett. 2023, 947, L20, [arXiv:...

2023 arXiv
[275]

Polarized X-Ray Emission from Magnetized Neutron Stars: Signature of Strong-Field Vacuum Polarization

Lai, D.; Ho, W.C. Polarized X-Ray Emission from Magnetized Neutron Stars: Signature of Strong-Field Vacuum Polarization. Phys. Rev. Lett. 2003, 91, 071101, [arXiv:astro-ph/astro-ph/0303596]. https://doi.org/10.1103/PhysRevLett.91.071101

2003 arXiv
[276]

eXTP: Enhanced X-ray Timing and Polarization mission

Zhang, S.N.; Feroci, M.; Santangelo, A.; Dong, Y.W.; Feng, H.; Lu, F.J.; Nandra, K.; Wang, Z.S.; Zhang, S.; Bozzo, E.; et al. eXTP: Enhanced X-ray Timing and Polarization mission. In Proceedings of the Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray; den He...

2016
[277]

Gamma-ray binaries and related systems

Dubus, G. Gamma-ray binaries and related systems. Astron. Astrophys. Rev. 2013, 21, 64, [arXiv:astro-ph.HE/1307.7083]. https://doi.org/10.1007/s00159-013-0064-5

2013 arXiv
[278]

PSR 1259-63: A Binary Radio Pulsar with a Be Star Companion

Johnston, S.; Manchester, R.N.; Lyne, A.G.; Bailes, M.; Kaspi, V .M.; Qiao, G.; D’Amico, N. PSR 1259-63: A Binary Radio Pulsar with a Be Star Companion. Astrophys. J. Lett. 1992, 387, L37. https://doi.org/10.1086/186300

1992 doi
[279]

Radio Detection of LAT PSRs J1741-2054 and J2032+4127: No Longer Just Gamma-ray Pulsars

Camilo, F.; Ray, P .S.; Ransom, S.M.; Burgay, M.; Johnson, T.J.; Kerr, M.; Gotthelf, E.V .; Halpern, J.P .; Reynolds, J.; Romani, R.W.; et al. Radio Detection of LAT PSRs J1741-2054 and J2032+4127: No Longer Just Gamma-ray Pulsars. Astrophys. J. 2009, 705, 1–13, [arXiv:astro-p...

2009 arXiv
[280]

A multimission catalogue of ultraluminous X-ray source candidates

Walton, D.J.; Mackenzie, A.D.A.; Gully, H.; Patel, N.R.; Roberts, T.P .; Earnshaw, H.P .; Mateos, S. A multimission catalogue of ultraluminous X-ray source candidates. Mon. Not. R. Astron. Soc. 2022, 509, 1587–1604, [arXiv:astro-ph.HE/2110.07625]. https://doi.org/10.1093/mnras...

2022 arXiv
[281]

An ultraluminous X-ray source powered by an accreting neutron star

Bachetti, M.; Harrison, F.A.; Walton, D.J.; Grefenstette, B.W.; Chakrabarty, D.; Fürst, F.; Barret, D.; Beloborodov, A.; Boggs, S.E.; Christensen, F.E.; et al. An ultraluminous X-ray source powered by an accreting neutron star. Nature 2014, 514, 202–204, [arXiv:astro-ph.HE/141...

2014 arXiv
[282]

Discovery of Coherent Pulsations from the Ultraluminous X-Ray Source NGC 7793 P13

Fürst, F.; Walton, D.J.; Harrison, F.A.; Stern, D.; Barret, D.; Brightman, M.; Fabian, A.C.; Grefenstette, B.; Madsen, K.K.; Middleton, M.J.; et al. Discovery of Coherent Pulsations from the Ultraluminous X-Ray Source NGC 7793 P13. Astrophys. J. Lett. 2016, 831, L14, [arXiv:as...

2016 arXiv
[283]

An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907

Israel, G.L.; Belfiore, A.; Stella, L.; Esposito, P .; Casella, P .; De Luca, A.; Marelli, M.; Papitto, A.; Perri, M.; Puccetti, S.; et al. An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907. Science 2017, 355, 817–819, [arXiv:astro-ph...

2017 arXiv
[284]

Discovery of a 0.42-s pulsar in the ultraluminous X-ray source NGC 7793 P13

Israel, G.L.; Papitto, A.; Esposito, P .; Stella, L.; Zampieri, L.; Belfiore, A.; Rodríguez Castillo, G.A.; De Luca, A.; Tiengo, A.; Haberl, F.; et al. Discovery of a 0.42-s pulsar in the ultraluminous X-ray source NGC 7793 P13. Mon. Not. R. Astron. Soc. 2017, 466, L48–L52, [a...

2017 arXiv
[285]

Discovery of pulsations from NGC 300 ULX1 and its fast period evolution

Carpano, S.; Haberl, F.; Maitra, C.; Vasilopoulos, G. Discovery of pulsations from NGC 300 ULX1 and its fast period evolution. Mon. Not. R. Astron. Soc. 2018, 476, L45–L49, [arXiv:astro-ph.HE/1802.10341]. https://doi.org/10.1093/mnrasl/sly030

2018 arXiv
[286]

The discovery of weak coherent pulsations in the ultraluminous X-ray source NGC 1313 X-2

Sathyaprakash, R.; Roberts, T.P .; Walton, D.J.; Fuerst, F.; Bachetti, M.; Pinto, C.; Alston, W.N.; Earnshaw, H.P .; Fabian, A.C.; Middleton, M.J.; et al. The discovery of weak coherent pulsations in the ultraluminous X-ray source NGC 1313 X-2. Mon. Not. R. Astron. Soc. 2019, ...

2019 arXiv
[287]

Discovery of a 2.8 s Pulsar in a 2 Day Orbit High-mass X-Ray Binary Powering the Ultraluminous X-Ray Source ULX-7 in M51

Rodríguez Castillo, G.A.; Israel, G.L.; Belfiore, A.; Bernardini, F.; Esposito, P .; Pintore, F.; De Luca, A.; Papitto, A.; Stella, L.; Tiengo, A.; et al. Discovery of a 2.8 s Pulsar in a 2 Day Orbit High-mass X-Ray Binary Powering the Ultraluminous X-Ray Source ULX-7 in M51. ...

2020 arXiv
[288]

A 78 Day X-Ray Period Detected from NGC 5907 ULX1 by Swift

Walton, D.J.; Fürst, F.; Bachetti, M.; Barret, D.; Brightman, M.; Fabian, A.C.; Gehrels, N.; Harrison, F.A.; Heida, M.; Middleton, M.J.; et al. A 78 Day X-Ray Period Detected from NGC 5907 ULX1 by Swift. Astrophys. J. Lett. 2016, 827, L13, [arXiv:astro- ph.HE/1607.07448]. http...

2016 arXiv
[289]

Swift Monitoring of M51: A 38 day Superorbital Period for the Pulsar ULX7 and a New Transient Ultraluminous X-Ray Source

Brightman, M.; Earnshaw, H.; Fürst, F.; Harrison, F.A.; Heida, M.; Israel, G.; Pike, S.; Stern, D.; Walton, D.J. Swift Monitoring of M51: A 38 day Superorbital Period for the Pulsar ULX7 and a New Transient Ultraluminous X-Ray Source. Astrophys. J. 2020, 895, 127, [arXiv:astro...

2020 arXiv
[290]

A mass of less than 15 solar masses for the black hole in an ultraluminous X-ray source

Motch, C.; Pakull, M.W.; Soria, R.; Grisé, F.; Pietrzy ´ nski, G. A mass of less than 15 solar masses for the black hole in an ultraluminous X-ray source. Nature 2014, 514, 198–201, [arXiv:astro-ph.HE/1410.4250]. https://doi.org/10.1038/nature13730

2014 arXiv
[291]

Swift Detection of a 65 Day X-Ray Period from the Ultraluminous Pulsar NGC 7793 P13

Hu, C.P .; Li, K.L.; Kong, A.K.H.; Ng, C.Y.; Lin, L.C.C. Swift Detection of a 65 Day X-Ray Period from the Ultraluminous Pulsar NGC 7793 P13. Astrophys. J. Lett. 2017, 835, L9, [arXiv:astro-ph.HE/1701.02449]. https://doi.org/10.3847/2041-8213/835/1/L9

2017 arXiv
[292]

ULX spectra revisited: Accreting, highly magnetized neutron stars as the engines of ultraluminous X-ray sources

Koliopanos, F.; Vasilopoulos, G.; Godet, O.; Bachetti, M.; Webb, N.A.; Barret, D. ULX spectra revisited: Accreting, highly magnetized neutron stars as the engines of ultraluminous X-ray sources. Astron. Astrophys. 2017, 608, A47, [arXiv:astro- ph.HE/1710.04953]. https://doi.or...

2017 arXiv
[293]

Evidence for Precession due to Supercritical Accretion in Ultraluminous X-Ray Sources

Weng, S.S.; Feng, H. Evidence for Precession due to Supercritical Accretion in Ultraluminous X-Ray Sources. Astrophys. J. 2018, 853, 115, [arXiv:astro-ph.HE/1712.09536]. https://doi.org/10.3847/1538-4357/aaa45c

2018 arXiv
[294]

On the maximum accretion luminosity of magnetized neutron stars: connecting X-ray pulsars and ultraluminous X-ray sources

Mushtukov, A.A.; Suleimanov, V .F.; Tsygankov, S.S.; Poutanen, J. On the maximum accretion luminosity of magnetized neutron stars: connecting X-ray pulsars and ultraluminous X-ray sources. Mon. Not. R. Astron. Soc. 2015, 454, 2539–2548, [arXiv:astro-ph.HE/1506.03600]. https://...

2015 arXiv
[295]

The ultraluminous X-ray source NuSTAR J095551+6940.8: a magnetar in a high-mass X-ray binary

Eksi, K.Y.; Andac, I.C.; Cikintoglu, S.; Gencali, A.A.; Gungor, C.; Oztekin, F. The ultraluminous X-ray source NuSTAR J095551+6940.8: a magnetar in a high-mass X-ray binary. Mon. Not. R. Astron. Soc. 2015, 448, L40–L42, [arXiv:astro- ph.HE/1410.5205]. https://doi.org/10.1093/m...

2015 arXiv
[296]

An accreting low magnetic field magnetar for the ultraluminous X-ray source in M82

Tong, H. An accreting low magnetic field magnetar for the ultraluminous X-ray source in M82. Research in Astronomy and Astrophysics 2015, 15, 517, [arXiv:astro-ph.HE/1411.3168]. https://doi.org/10.1088/1674-4527/15/4/005

2015 arXiv
[297]

No magnetars in ULXs

King, A.; Lasota, J.P . No magnetars in ULXs. Mon. Not. R. Astron. Soc. 2019, 485, 3588–3594, [arXiv:astro-ph.HE/1903.03624]. https://doi.org/10.1093/mnras/stz720

2019 arXiv
[298]

On the Magnetic Fields, Beaming Fractions, and Fastness Parameters of Pulsating Ultraluminous X-Ray Sources

Erkut, M.H.; Türko˘ glu, M.M.; Ek¸ si, K.Y.; Alpar, M.A. On the Magnetic Fields, Beaming Fractions, and Fastness Parameters of Pulsating Ultraluminous X-Ray Sources. Astrophys. J. 2020, 899, 97, [arXiv:astro-ph.HE/2007.08102]. https://doi.org/10.3847/15 38-4357/aba61b

2020 arXiv
[299]

Magnetic field strength of a neutron-star-powered ultraluminous X-ray source

Brightman, M.; Harrison, F.A.; Fürst, F.; Middleton, M.J.; Walton, D.J.; Stern, D.; Fabian, A.C.; Heida, M.; Barret, D.; Bachetti, M. Magnetic field strength of a neutron-star-powered ultraluminous X-ray source. Nature Astronomy 2018, 2, 312–316, [arXiv:astro- ph.HE/1803.02376...

2018 arXiv
[300]

A Potential Cyclotron Resonant Scattering Feature in the Ultraluminous X-Ray Source Pulsar NGC 300 ULX1 Seen by NuSTAR and XMM-Newton

Walton, D.J.; Bachetti, M.; Fürst, F.; Barret, D.; Brightman, M.; Fabian, A.C.; Grefenstette, B.W.; Harrison, F.A.; Heida, M.; Kennea, J.; et al. A Potential Cyclotron Resonant Scattering Feature in the Ultraluminous X-Ray Source Pulsar NGC 300 ULX1 Seen by NuSTAR and XMM-Newt...

2018 arXiv

Pith tools

Reviewed August 11, 2026 · model on record in the stance chip above.

[1] [1]

Evidence for x Rays From Sources Outside the Solar System

Giacconi, R.; Gursky, H.; Paolini, F.R.; Rossi, B.B. Evidence for x Rays From Sources Outside the Solar System. Phys. Rev. Lett. 1962, 9, 439–443. https://doi.org/10.1103/PhysRevLett.9.439

doi:10.1103/physrevlett.9.439 1962

[2] [2]

X-Ray Binaries

Casares, J.; Jonker, P .G.; Israelian, G. X-Ray Binaries. InHandbook of Supernovae; Alsabti, A.W.; Murdin, P ., Eds.; 2017; p. 1499. https://doi.org/10.1007/978-3-319-21846-5_111

work page doi:10.1007/978-3-319-21846-5_111 2017

[3] [3]

Accreting Binaries; Nature, formation, and evolution; 2022

Chaty, S. Accreting Binaries; Nature, formation, and evolution; 2022. https://doi.org/10.1088/2514-3433/ac595f

doi:10.1088/2514-3433/ac595f 2022

[4] [4]

The Milky Way in X-rays for an outside observer

Grimm, H.J.; Gilfanov, M.; Sunyaev, R. The Milky Way in X-rays for an outside observer. Log(N)-Log(S) and luminosity function of X-ray binaries from RXTE/ASM data. Astron. Astrophys. 2002, 391, 923–944, [arXiv:astro-ph/astro-ph/0109239]. https://doi.org/10.1051/0004-6361:20020826

arXiv 2002

[5] [5]

BlackCAT: A catalogue of stellar-mass black holes in X-ray transients

Corral-Santana, J.M.; Casares, J.; Muñoz-Darias, T.; Bauer, F.E.; Martínez-Pais, I.G.; Russell, D.M. BlackCAT: A catalogue of stellar-mass black holes in X-ray transients. Astron. Astrophys. 2016, 587, A61, [arXiv:astro-ph.HE/1510.08869]. https: //doi.org/10.1051/0004-6361/201527130

arXiv 2016

[6] [6]

X-Ray Properties of Black-Hole Binaries

Remillard, R.A.; McClintock, J.E. X-Ray Properties of Black-Hole Binaries. Annu. Rev. Astron. Astrophys. 2006, 44, 49–92, [arXiv:astro-ph/astro-ph/0606352]. https://doi.org/10.1146/annurev.astro.44.051905.092532

arXiv 2006

[7] [7]

Modelling the behaviour of accretion flows in X-ray binaries

Done, C.; Gierli ´ nski, M.; Kubota, A. Modelling the behaviour of accretion flows in X-ray binaries. Everything you always wanted to know about accretion but were afraid to ask. Astron. Astrophys. Rev. 2007, 15, 1–66, [arXiv:astro-ph/0708.0148]. https://doi.org/10.1007/s00159-007-0006-1

arXiv 2007

[8] [8]

Low-Mass X-ray Binaries

Bahramian, A.; Degenaar, N. Low-Mass X-ray Binaries. In Handbook of X-ray and Gamma-ray Astrophysics ; 2023; p. 120. https://doi.org/10.1007/978-981-16-4544-0_94-1

doi:10.1007/978-981-16-4544-0_94-1 2023