Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-11-09
Astronomy and Astrophysics
Astrophysics
6 pages, 2 figures; Proceedings of the ESO Workshop on "Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography a
Scientific paper
Black hole X-ray binaries are transient probably because their discs are subject to the same thermal-viscous instability which is present in dwarf nova binary systems. I discuss applications of the dwarf-nova instability model to transient, low-mass, X-ray binary systems. When disc truncation and X-ray irradiation are taken into account this model is capable of reproducing the basic properties of X-ray binary outbursts (Dubus et al. 2000).
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