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The Temperatures of White Dwarfs in Dwarf Novae

Published online by Cambridge University Press:  12 April 2016

B. J. M. Hassall  and
C. La Dous
B. J. M. Hassall
Affiliation:
Centre for Astrophysics, University of Central Lancashire, Preston, PR1 2HE, UK
C. La Dous
Affiliation:
ESA/IUE Observatory, Villafranca del Castillo, Apartado 50727, 28080 Madrid, Spain

Abstract

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We attempt to measure the temperature of all the quiescent dwarf novae that have been observed with IUE, by fitting the observed flux distribution of white dwarfs (WDs) with known temperatures. This approach gives results similar to those using much more sophisticated modelling, but allows us to investigate the relationship with system parameters and subclasses.

Type
Non-Magnetic Cataclysmic Variables
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 85 - 86
Copyright
Copyright © Kluwer 1996

References

Horne, K., Marsh, T.R., Cheng, F.H., et al., 1994, Ap. J., 426, 294 Google Scholar
la Dous, C., 1996, in preparation.Google Scholar