Results 21 to 30 of about 418,649 (286)
Why Do Black--Hole X-ray Binaries Tend to Be Transient? [PDF]
, 1999 Black hole X-ray binaries are transient probably because their discs are subject to the same thermal-viscous instability which is present in dwarf nova binary systems.
Lasota, Jean-Pierre
core +3 more sources
Beam Pattern Evolution of Accreting X-Ray Pulsar 1A 0535+262 during Its 2020 Giant Outburst
The Astrophysical Journal, 2023 We report on pulse profile decomposition analysis of bright transient X-ray pulsar 1A 0535+262 using broadband Insight-HXMT observations during a giant outburst of the source in 2020.
Y. F. Hu +9 more
doaj +1 more source
Faint Galactic X-ray Binaries [PDF]
AIP Conference Proceedings, 2008 8 pages, published in the proceedings of "A population Explosion", AIP Conference Proceedings Volume 1010, pp.
Jonker, P. G. +6 more
openaire +2 more sources
Back to Business: SLX 1746–331 after 13 Years of Silence
The Astrophysical Journal, 2023 The black hole candidate system SLX 1746–331 was back to business in 2023, after a long silence of roughly 13 years. An outburst was observed thoroughly by Insight-HXMT and NICER.
Jing-Qiang Peng +19 more
doaj +1 more source
, 2023 Invited chapter for Handbook of X-ray and Gamma-ray Astrophysics, 44 pages of text, 11 pages of references, 18 figures, 1 ...
Fornasini, Francesca M. +2 more
openaire +2 more sources
Generation of X-Ray Fluctuations in X-Ray Binaries [PDF]
International Astronomical Union Colloquium, 1996 AbstractShort-term aperiodic fluctuations with 1/f-like power spectral density (PSD), where f is the frequency, are characteristics of X-ray radiation from X-ray binaries. To investigate a mechanism creating fluctuations, we construct a cellular-automaton model for accretion disks based on the concept of self organized criticality (SOC). In this model,
S. Mineshige, M. Takeuchi, H. Negoro
openaire +1 more source
X-RAY POLARIZATION FROM HIGH-MASS X-RAY BINARIES [PDF]
The Astrophysical Journal, 2015 X-ray astronomy allows study of objects which may be associated with compact objects, i.e. neutron stars or black holes, and also may contain strong magnetic fields. Such objects are categorically non-spherical, and likely non-circular when projected on the sky.
T. Kallman, A. Dorodnitsyn, J. Blondin
openaire +2 more sources
The Astrophysical Journal, 2023 Observations of the high-mass gamma-ray binary LS 2883/PSR B1259–63 with the Chandra X-ray Observatory during the 2011–2014 and 2014–2017 binary cycles have shown X-ray-emitting clumps, presumably ejected from the binary during periastron passages. These
Jeremy Hare +3 more
doaj +1 more source
Populating the Galaxy with low-mass X-ray binaries [PDF]
, 2006 We perform binary population synthesis calculations to investigate the incidence of low-mass X-ray binaries and their birth rate in the Galaxy. We use a binary evolution algorithm that models all the relevant processes including tidal circularization and
Hurley, Jarrod R., Kiel, Paul D.
core +3 more sources
The eclipsing X-ray pulsar X-7 in M33 [PDF]
, 1998 Using our extensive ROSAT X-ray observations of M33, we confirm a 3.45 day eclipse period for the Einstein source X-7 (Larson & Schulman, 1997) and discover evidence for a 0.31-s pulse period.
Brazier +25 more
core +3 more sources