New types of X-ray flares/bursts from GRS 1915+105

Details New types of X-ray flares/bursts from GRS 1915+105 New types of X-ray flares/bursts from GRS 1915+105

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.459..399y&link_type=abstract

In: Exploring the gamma-ray universe. Proceedings of the Fourth INTEGRAL Workshop, 4-8 September 2000, Alicante, Spain. Editor:

Physics

Black Hole, X-Ray Binary, X-Ray Bursts

Scientific paper

We present results of different types of X-ray flares/bursts observed in GRS 1915+105 lasting from 30 s to 1300 s from the analysis of RXTE/PPC data. Each burst consists of a low flux quiescent phase followed by a high flux burst phase. All the observed bursts have a slow exponential rise, a sharp linear decay, and are harder during the burst phase. The 13-60 keV flux relative to 2-13 keV flux is higher during the quiescent phase than that during the burst phase. For all the observed bursts, the duration of quiescent phase is inversely proportional to the square of the QPO frequency (2-10 Hz).

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