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arXiv · astro-ph/0105478

X-Ray Bursts from the Galactic X-Ray Transient Source GRS 1915+105

J. S. Yadav·A. R. Rao
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Abstract

We have analyzed publicly available RXTE/PCAs archival data of GRS 1915+105 during its burst/flaring state. The burst cycle ranges from 30 to 1300 s. These bursts are different from the type I and type II classical bursts seen in Low Mass X-ray Binaries (LMXBs) in terms of their temporal and spectral properties. We have classified these bursts on the basis of properties observed during the quiescent (low flux) phase. The 2 - 10 Hz QPOs are present during the quiescent phase and disappear during the burst phase of all types of these X-ray bursts. The duration of the quiescent phase can be explained assuming an outflow from the post-shock regions and the catastrophic Compton cooling.

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J. S. Yadav, A. R. Rao. 2001-05-28. X-Ray Bursts from the Galactic X-Ray Transient Source GRS 1915+105. https://doi.org/10.1016/s0273-1177(01)00433-1

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