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Physics of Mass Ejection During Nova Outbursts

Published online by Cambridge University Press:  12 April 2016

Mariko Kato
Mariko Kato*
Affiliation:
Department of Astronomy, Keio University, Hiyoshi, Kouhoku-ku, Yokohama 223Japan

Abstract

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During nova outbursts a large part of the envelope mass is blown off. This mass ejection is caused mainly by the radiation driven wind and by the Roche lobe overflow. Theoretical studies on the acceleration mechanisms are briefly reviewed. Finally, I present theoretical light curves for U Sco based on the steady wind approach.

Type
2. Models of Observations
Information
International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 236 - 243
Copyright
Copyright © Springer-Verlag 1990

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