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Theoretical Light Curves of Recurrent Novae

Published online by Cambridge University Press:  07 August 2017

M. Kato
M. Kato*
Affiliation:
Department of Astronomy, Keio University, Yokohama 223, Japan

Abstract

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Theoretical light curves for the decay phase of recurrent novae are obtained using optically thick wind theory. With the OPAL opacity tables the decay time scale is drastically shortened.

Type
IV. Planetary Nebulae Connection: Evolution from the AGB
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 408
Copyright
Copyright © Kluwer 1993