Spectral fitting of 2022 observations indicates the disk reaches 7-17 R_g from the neutron star at low inclination, with first reported type-II bursts attributed to magnetospheric gating.
year = 1993, month = sep, volume =
12 Pith papers cite this work. Polarity classification is still indexing.
12
Pith papers citing it
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astro-ph.HE 12representative citing papers
Candidate mHz QPOs detected in GX 3+1 at 7-15 mHz with 0.51-1.41% rms, one surviving global significance, occurring at higher luminosities than in other NS LMXBs.
A new relativistic model for accretion-powered X-ray pulsars enables simultaneous computation of phase-averaged spectra and pulse profiles, applied to NuSTAR data for Her X-1 to extract physical parameters and beaming patterns.
New observations of 4U 1323-62 detect 12 bursts, confirm 2.94-hour dips, a 0.9 Hz QPO, and suggest a ~10-year cyclic variation in burst rate.
Marginal X-ray polarization detection in atoll source 4U 1735-44 is consistent with a low disk inclination of about 40 degrees inferred from relativistic reflection modeling.
Simultaneous X-ray and optical observation of a type I burst in EXO 0748-676 shows a 4.46 s optical lag after 16 years of quiescence.
Observations show a long thermonuclear burst in MAXI J0911--655 followed by a flare interpreted as burst-driven thermal-viscous disk instability enhancing accretion.
Observational analysis of type-II bursts in MXB 1730-335 confirms mode-dependent power-law relations between burst fluence and recurrence time plus a critical fluence threshold for peak-flux correlation.
XSPECT observations of two soft X-ray transients during outburst decay reveal superburst evolution with cooling blackbody emission and a flux-dependent hardening of Comptonized spectra.
Significant X-ray flux blocking in 4U 1746-37 allows the neutron star to have canonical mass and radius values of 1.59 solar masses and 13 km or 2.12 solar masses and 9.8 km.
NuSTAR and NICER data on SAX J1808.4-3658 show the accretion disk truncating to ~23 R_g in 2025 with magnetospheric radius exceeding co-rotation radius, indicating a possible transition to the propeller regime while accretion continues as evidenced by a Type-I burst.
Discovery of an eclipsing neutron star LMXB with clocked bursts, orbital period 6.483 hr, companion mass 0.6-0.8 Msun, and helium burst indications from energy ratio 120-130.
citing papers explorer
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On the assessment of the disk truncation and detection of type-II bursts from the accreting millisecond X-ray Pulsar IGR J17062-6143
Spectral fitting of 2022 observations indicates the disk reaches 7-17 R_g from the neutron star at low inclination, with first reported type-II bursts attributed to magnetospheric gating.
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Evidence for Millihertz Oscillations in the bright atoll source GX 3+1
Candidate mHz QPOs detected in GX 3+1 at 7-15 mHz with 0.51-1.41% rms, one surviving global significance, occurring at higher luminosities than in other NS LMXBs.
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A New Relativistic Model for Spectral Formation in Accretion-Powered X-ray Pulsars: Pulse Profiles and Phase-Averaged Spectra
A new relativistic model for accretion-powered X-ray pulsars enables simultaneous computation of phase-averaged spectra and pulse profiles, applied to NuSTAR data for Her X-1 to extract physical parameters and beaming patterns.
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A Cyclic Burst Rate Behavior of a Persistent X-ray Burster: Recent XMM-Newton and NuSTAR Observations of 4U 1323-62
New observations of 4U 1323-62 detect 12 bursts, confirm 2.94-hour dips, a 0.9 Hz QPO, and suggest a ~10-year cyclic variation in burst rate.
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X-Ray Polarization from the Atoll 4U 1735-44 Suggests a Low Inclination
Marginal X-ray polarization detection in atoll source 4U 1735-44 is consistent with a low disk inclination of about 40 degrees inferred from relativistic reflection modeling.
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Simultaneous Optical and X-ray Detection of a Thermonuclear Burst in the 2024 Outburst of EXO 0748-676
Simultaneous X-ray and optical observation of a type I burst in EXO 0748-676 shows a 4.46 s optical lag after 16 years of quiescence.
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Long thermonuclear burst driven thermal-viscous instability of accretion disk: triggering an outburst-like X-ray flare
Observations show a long thermonuclear burst in MAXI J0911--655 followed by a flare interpreted as burst-driven thermal-viscous disk instability enhancing accretion.
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Statistical properties of type-II bursts in Rapid Burster observed with Insight-HXMT
Observational analysis of type-II bursts in MXB 1730-335 confirms mode-dependent power-law relations between burst fluence and recurrence time plus a critical fluence threshold for peak-flux correlation.
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Tracing the outburst decay of soft X-ray transients Aql X-1 and 4U 1608-52 with XSPECT
XSPECT observations of two soft X-ray transients during outburst decay reveal superburst evolution with cooling blackbody emission and a flux-dependent hardening of Comptonized spectra.
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The compact neutron star in 4U 1746-37 revisited: Reassessing the mass and radius
Significant X-ray flux blocking in 4U 1746-37 allows the neutron star to have canonical mass and radius values of 1.59 solar masses and 13 km or 2.12 solar masses and 9.8 km.
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Probing the accretion geometry of the transient accreting millisecond pulsar SAX J1808.4-3658: transitions to the propeller regime
NuSTAR and NICER data on SAX J1808.4-3658 show the accretion disk truncating to ~23 R_g in 2025 with magnetospheric radius exceeding co-rotation radius, indicating a possible transition to the propeller regime while accretion continues as evidenced by a Type-I burst.
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Einstein Probe discovery of EP J171159.4-333253: an eclipsing neutron star low-mass X-ray binary with clocked bursts
Discovery of an eclipsing neutron star LMXB with clocked bursts, orbital period 6.483 hr, companion mass 0.6-0.8 Msun, and helium burst indications from energy ratio 120-130.