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Mass loss from interacting close binary systems

Published online by Cambridge University Press:  12 April 2016

Mirek J. Plavec
Mirek J. Plavec*
Affiliation:
Department of Astronomy, University of California Los Angeles, CA 90024, U. S. A.

Abstract

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Mass outflow from interacting close binary systems, accompanied by loss of orbital angular momentum, appears to be a very important process affecting the evolution of binary stars. Together with accretion on the mass-gaining component, it is the least understood aspect of the general complex process we call “evolution with mass transfer and/or mass loss”, or, more briefly, “interaction”. It is therefore very imperative to assemble and examine all available facts or hints about mass loss.

Type
Session VIII - Effects of Mass Loss on the Evolution of Binary Stars
Information
International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 431 - 456
Copyright
Copyright © Reidel 1981

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