X-ray flares/bursts from GRS 1915+105 and the two component accretion flow

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dc.creatorYadav, J. S.
dc.creatorRao, A. R.
dc.date2001-05-29
dc.date.accessioned2026-07-07T01:58:42Z
dc.date.available2026-07-07T01:58:42Z
dc.descriptionWe 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 about 20 s (R1), 2) regular bursts with short quiescent phase of about 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).
dc.descriptionTo publish in Astrophysics and Space Science, Email: jsyadav@tifr.res.in
dc.identifierhttps://arxiv.org/abs/astro-ph/0105494
dc.identifierhttp://arxiv.org/abs/astro-ph/0105494
dc.identifierAstrophys.Space Sci. 276 (2001) 221-224
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2822
dc.subjectAstrophysics
dc.titleX-ray flares/bursts from GRS 1915+105 and the two component accretion flow
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