GLITCHES IN SOFT-X-RAY TRANSIENTS - ECHOES OF THE MAIN BURST

Citation
T. Augusteijn et al., GLITCHES IN SOFT-X-RAY TRANSIENTS - ECHOES OF THE MAIN BURST, Astronomy and astrophysics, 279(1), 1993, pp. 13-16
Citations number
22
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
00046361
Volume
279
Issue
1
Year of publication
1993
Pages
13 - 16
Database
ISI
SICI code
0004-6361(1993)279:1<13:GIST-E>2.0.ZU;2-L
Abstract
Several soft X-ray transients exhibit one or more intensity jumps (''g litches'') that interrupt the decay of the initial ''main'' burst. We interpret these glitches as due to enhanced mass flow from the compani on star which is responding, essentially linearly, to beating by X-ray s from the primary. The process goes on continuously, triggered by ('' echoing'') the initial burst. A time delay T of a few months occurs in the similarly linear flow of matter from the companion surface to the X-ray-emitting inner disk. The time scale in the inner disk is a few days. If this model is correct there is evidence that the main burst, that has been observed to decay over a time less than or similar to T, is caused by a burst of mass flow from the companion.