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Is There Observational Evidence for the Evaporation of the Inner Accretion Disk in Dwarf Novae at Quiescence?

Published online by Cambridge University Press:  12 April 2016

C. La Dous ,
E. Meyer-Hofmeister  and
F. Meyer
C. La Dous
Affiliation:
ESA/IUE Observatory, Villafranca del Castillo, Apartado 50727, 28080 Madrid, Spain
E. Meyer-Hofmeister
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85740 Garching, Germany
F. Meyer
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85740 Garching, Germany

Abstract

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We present the preliminary results of a comparison of observed general patterns of quiescent dwarf novae and theoretical predictions of the disk evaporation model. We demonstrate that, even though details still have to be clarified, on the whole there is strong evidence that observations and theory are in agreement.

Type
Non-Magnetic Cataclysmic Variables
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 81 - 84
Copyright
Copyright © Kluwer 1996

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