Microquasars pp 221-224 | Cite as

X-Ray Flares/Bursts from GRS 1915+105 and the Two Component Accretion Flow

  • J. S. Yadav
  • A. R. Rao
Conference paper


We present results of our analysis of a set of RXTE/PCA observations of X-ray flares/bursts with burst cycle ranging from 30 to 1300 s from the Galactic X-ray transient source GRS 1915+105 during last four years. These flares/bursts can be classified into four types: 1) regular bursts with short burst phase of ∼ 20 s (R1), 2) regular bursts with short quiescent phase of ∼ 20 s (R2), 3) long regular bursts (R3) with burst cycle ≥ 1000 s, and 4) irregular bursts (IR). For all the observed bursts, the duration of the quiescent phase is inversely proportional to the square of the QPO frequency (2–10 Hz).


Accretion Disk Burst Duration Quiescent Phase Burst Phase Vertical Branch 
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Copyright information

© Springer Science+Business Media New York 2001

Authors and Affiliations

  • J. S. Yadav
    • 1
  • A. R. Rao
    • 1
  1. 1.Tata Institute of Fundamental ResearchMumbaiIndia

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