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Observations of Dwarf Novae

Published online by Cambridge University Press:  14 August 2015

B. Warner
B. Warner*
Affiliation:
Dept. of Astronomy, University of Cape Town, South Africa

Abstract

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Spectroscopic and photometric observations relevant to the structure of classical novae, recurrent novae and dwarf novae are collected together. Details are given of optical, infrared, satellite ultraviolet, X-ray and radio observations. Most of these can be understood in terms of the hot spot model of cataclysmic variable stars. Estimates are made of luminosities, temperatures and rates of mass transfer. Observations made during eruptions of dwarf novae imply large changes taking place in the accretion disc.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 73: Structure and Evolution of Close Binary Systems , 1976 , pp. 85 - 140
Copyright
Copyright © Reidel 1976 

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