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The Implications of Disc Instabilities on Cataclysmic Variable Structure and Evolution

Published online by Cambridge University Press:  22 February 2018

J.-P. Lasota
J.-P. Lasota*
Affiliation:
Institut d'Astrophysique de Paris, France

Abstract

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Applications of the thermal-viscous disc instability model to various classes of cataclysmic variable very often require the accretion disc to be truncated. I argue that in most cases this inner truncation must be due to the white dwarf's magnetic field.

Resumen

Resumen

Al aplicar el modelo de inestabilidad ténnieo-viscosa del disco a varias clases de variables catacíismicas, con frecuencia se requiere que el disco de aereción sea truncado. Arguyo que en la mayoría de los casos este truncamiento interno se debe al campo magnético de la enana blanca.

Keywords

AccretionAccretion Discs — Instabilities — NovaeCataclysmic Variables — Stars: Evolution
Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 124 - 127
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

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