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The Nova-Like Variables

Published online by Cambridge University Press:  12 April 2016

Vik Dhillon
Vik Dhillon*
Affiliation:
Royal Greenwich Observatory, La Palma

Abstract

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We review optical observations and theoretical models of the non-magnetic nova-like variables (UX UMa, VY Scl and SW Sex stars). A brief discussion of the classification scheme is followed by a statistical overview of the observed properties. The most important features of each of the sub-classes are then reviewed, concluding with a summary of the theoretical models invoked to understand these systems.

Information

Type
Non-Magnetic Cataclysmic Variables
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996, pp. 3 - 12
Copyright
Copyright © Kluwer 1996

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