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Gravitational Radiation and the Evolution of Low Mass Binaries∗

Published online by Cambridge University Press:  14 August 2015

John Faulkner
John Faulkner*
Affiliation:
Lick Observatory, Board of Studies in Astronomy and Astrophysics, University of California, Santa Cruz, Calif. 95064, U.S.A.

Abstract

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Gravitational radiation of energy and angular momentum can modify and in some cases, control the evolution of a close binary system. The region of interest is briefly delineated. Recent work of the author and colleagues of relevance to this area is discussed, including theoretical studies of accretion, mass loss and mass transfer, and an observational study of a system, HZ 29 where gravitational radiation may dictate its behaviour.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 73: Structure and Evolution of Close Binary Systems , 1976 , pp. 193 - 204
Copyright
Copyright © Reidel 1976 

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