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Title:
Long time-scale variability in GRS 1915+105
Authors:
Truss, M. R.; Wynn, G. A.
Affiliation:
AA(School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS), AB(Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH)
Publication:
Monthly Notices of the Royal Astronomical Society, Volume 353, Issue 4, pp. 1048-1054. (MNRAS Homepage)
Publication Date:
10/2004
Origin:
MNRAS
Astronomy Keywords:
accretion, accretion discs, binaries: close, stars: individual: GRS 1915+105
DOI:
10.1111/j.1365-2966.2004.08153.x
Bibliographic Code:
2004MNRAS.353.1048T

Abstract

We present very high resolution hydrodynamical simulations of accretion discs in black hole X-ray binaries accreting near the Eddington limit. The results show that mass loss, irradiation and tidal interactions all have a profound effect on the observed behaviour of long-period X-ray transients. In particular, the interplay of all of these effects in the outer regions of the accretion disc is able to drive long time-scale (weeks to years) variability is these objects, and is a possible origin for some of the extreme variability of GRS 1915+105.

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