REVIEW 6 cited by
Accreting Millisecond X-Ray Pulsars
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
Accreting Millisecond X-Ray Pulsars (AMXPs) are astrophysical laboratories without parallel in the study of extreme physics. In this chapter we review the past fifteen years of discoveries in the field. We summarize the observations of the fifteen known AMXPs, with a particular emphasis on the multi-wavelength observations that have been carried out since the discovery of the first AMXP in 1998. We review accretion torque theory, the pulse formation process, and how AMXP observations have changed our view on the interaction of plasma and magnetic fields in strong gravity. We also explain how the AMXPs have deepened our understanding of the thermonuclear burst process, in particular the phenomenon of burst oscillations. We conclude with a discussion of the open problems that remain to be addressed in the future.
Forward citations
Cited by 6 Pith papers
-
Relativistic X-ray reflection and thermonuclear burst from accreting millisecond X-ray pulsar SRGA J144459.2-604207
Time-resolved X-ray spectral fits of SRGA J1444 reveal up to 30% disk reflection during thermonuclear bursts, an inner disk radius near 11 gravitational radii, and a polar magnetic field around 6e8 Gauss.
-
Gravitational waves from r-mode oscillations of stochastically accreting neutron stars
Stochastic accretion impacts excite neutron star r-modes with root-mean-square GW strain near 1e-35 at 10 Hz, too weak for LIGO, plus an autocorrelation diagnostic for CFS instability.
-
Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes
Polarized X-ray pulse simulations show IXPE can constrain pulsar inclination and spot colatitude to a few degrees only for bright, small hot spots, and cannot distinguish circular from ring-like spot shapes.
-
A Detailed Spectral Study of Intermittent-Accreting Millisecond X-ray Pulsar Aql X-1 during Pulse-on and Pulse-off Stages
Phase-resolved spectroscopy of the intermittent X-ray pulsar Aql X-1 finds a soft excess in the pulse-high phase that the authors attribute to a small surface hotspot.
-
AstroSat timing and spectral analysis of the accretion-powered millisecond X-ray pulsar IGR J17591--2342
AstroSat timing and spectral analysis of IGR J17591-2342 confirms a 527.4 Hz spin, updates orbital parameters, and finds constant pulse amplitude with energy and soft X-ray phase lags.
-
Astrophysics with Compact Objects: An Indian Perspective, Present Status and Future Vision
A community-authored review of Indian compact-object astrophysics and a proposed roadmap for future investment in facilities, theory, and workforce.
Discussion (0). Continue with ORCID to comment.