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Disc Instabilities and “Soft” X-Ray Transients

Published online by Cambridge University Press:  12 April 2016

J.P. Lasota
J.P. Lasota*
Affiliation:
UPR 176 du CNRS, DARC, Observatoire de Paris, Section de Meudon, F–92195 Meudon Cedex, France

Abstract

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I review several problems which arise when one tries to apply the standard dwarf nova instability model to outbursts of soft X-ray transients

Type
Part 8. X-Ray Binaries, Transients and Super-Soft Sources
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 351 - 360
Copyright
Copyright © Astronomical Society of the Pacific 1997

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