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Generalized Theory of Shell Flash and Accreting White Dwarfs

Published online by Cambridge University Press:  14 August 2015

Daiichiro Sugimoto  and
Shigeki Miyaji
Daiichiro Sugimoto
Affiliation:
College of General Education, University of Tokyo Tokyo 153, Japan
Shigeki Miyaji
Affiliation:
College of General Education, University of Tokyo Tokyo 153, Japan

Abstract

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Shell flashes take place both in deep interior of red giant stars and near surface of accreting white dwarfs. Theories of shell flashes have been thus far presented piece by piece in different papers. It is the purpose of the present review to construct and generalize them in order to reach better understanding. A non-linear yet almost analytical theory is presented which treats the development of the shell flash in finite amplitude. Recurrence of the shell flashes is also shown to be well understood as a non-linear oscillation in dissipative system which tends to be its limit cycle. As a result strength of the peak energy-generation and recurrence time of the shell flashes are related with mass of the accreting white dwarfs, accretion rate, etc.

Type
Session 5: Mass-Accretion onto Compact Stars and Resultant Explosive Phenomena and Nucleosynthesis
Information
Symposium - International Astronomical Union , Volume 93: Fundamental Problems in the Theory of Stellar Evolution , 1981 , pp. 191 - 206
Copyright
Copyright © Reidel 1981 

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