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The Origin and Evolution of Novae

Published online by Cambridge University Press:  12 April 2016

A.V. Tutukov  and
L.R. Yungelson
A.V. Tutukov
Affiliation:
Astronomical Council of the USSR Academy of Science
L.R. Yungelson
Affiliation:
Astronomical Council of the USSR Academy of Science

Abstract

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The cataclysmic binaries are products of the nonconservative evolution of close binaries with large initial mass ratios of components. The accretors in cataclysmic binaries can be helium or carbon-oxygen or oxygen-neon-magnesium white dwarfs. Their annual birthrates are ~0.005, ~0.005, and ~0.00005 respectively. In one-zone approximation of a thin accreting shell we estimate the critical masses of hydrogen and helium shells and recurrence time scales of thermonuclear runaways.

Type
3. Theory
Information
International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 325 - 341
Copyright
Copyright © Springer-Verlag 1990

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