Orbital Period and Outburst Luminosity of Transient Low Mass X-ray Binaries

@article{Wu2010OrbitalPA,
  title={Orbital Period and Outburst Luminosity of Transient Low Mass X-ray Binaries},
  author={Ying Xiang Wu and W. D. Yu and T. P. Li and Thomas J. Maccarone and Xiang Dong Li},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2010}
}
  • Y. Wu, W. Yu, +2 authors X. Li
  • Published 1 June 2010
  • Physics
  • arXiv: High Energy Astrophysical Phenomena
In this paper we investigate the relation between the maximal luminosity of X-ray outburst and the orbital period in transient low mass X-ray binaries (or soft X-ray transients) observed by the Rossi X-ray Timing Explorer (RXTE) in the past decade. We find that the maximal luminosity (3-200 keV) in Eddington unit generally increases with increasing orbital period, which does not show a luminosity saturation but in general agrees with theoretical prediction. The peak luminosities in ultra… Expand

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References

SHOWING 1-10 OF 71 REFERENCES
State Transitions in Bright Galactic X-ray Binaries: Luminosities Span by Two Orders of Magnitude
Using X-ray monitoring observations with the All-Sky Monitor on board the Rossi X-Ray Timing Explorer and the Burst Alert Telescope on board the Swift, we are able to study the spectral stateExpand
Why soft X-ray transients can remain in the low/hard state during outburst
In the canonical understanding of transient X-ray sources the accretion during quiescence occurs via a geometrically thin disk in the outer part and via an advection-dominated hot coronal flow/ADAFExpand
The Properties of X-Ray and Optical Light Curves of X-Ray Novae
We have collected the available data from the literature and from public data archives covering the past two decades for the long-term X-ray and optical light curves of X-ray nova (XN) outbursts. XNExpand
The Correlation between Hard X-Ray Peak Flux and Soft X-Ray Peak Flux in the Outburst Rise of Low-Mass X-Ray Binaries
We have analyzed Rossi X-Ray Timing Explorer pointed observations of the outbursts of black hole and neutron star soft X-ray transients in which an initial low/hard state, or ``island'' state,Expand
Peak Luminosities of the Hard States of GX 339-4: Implications for the Accretion Geometry, Disk Mass, and Black Hole Mass
We have analyzed observations of the black hole transient GX 339-4 made with the Rossi X-ray Timing Explorer (RXTE) and the Burst and Transient Source Experiment (BATSE) on board the ComptonExpand
BLACK HOLE AND NEUTRON STAR TRANSIENTS IN QUIESCENCE
We consider the X-ray luminosity difference between neutron star and black hole soft X-ray transients (NS and BH SXTs) in quiescence. The current observational data suggest that BH SXTs areExpand
SPECTRAL AND TIMING EVOLUTION OF THE BLACK HOLE X-RAY NOVA 4U 1543-47 DURING ITS 2002 OUTBURST
We present an X-ray spectral and timing analysis of 4U 1543-47 during its 2002 outburst based on 49 pointed observations obtained using the Rossi X-ray Timing Explorer (RXTE). The outburst reached aExpand
The light curves of soft X‐ray transients
We show that the light curves of soft X-ray transients (SXTs) follow naturally from the disc instability picture, adapted to take account of irradiation by the central X-ray source during theExpand
Discovery of the accretion-powered millisecond pulsar swift j1756.9-2508 with a low-mass companion
We report on the discovery by the Swift Gamma-Ray Burst Explorer of the eighth known transient accretion-powered millisecond pulsar, SWIFT J1756.9-2508, as part of routine observations with the SwiftExpand
Complete RXTE Spectral Observations of the Black Hole X-ray Nova XTE J1550–564
We report on the X-ray spectral behavior of XTE J1550(564 during its 1998¨1999 outburst. XTE J1550(564 is an exceptionally bright X-ray nova and is also the third Galactic black hole candi- dateExpand
...
1
2
3
4
5
...