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Mass Loss and Shell Masses of Close Binary Stars

Published online by Cambridge University Press:  12 April 2016

V.G. Karetnikov
V.G. Karetnikov*
Affiliation:
Astronomical Department of the Odessa State University, Odessa, U.S.S.R.

Abstract

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From the values of period changes for 6 close binary stars the mass transfer rate was calculated. Comparing these values Mt with the values of shell masses Msh, the expression

was derived. The analysis of this expression points out the initial character of the outflow of matter, and one may determine the time interval of the substitution of the shell matter. So one may conclude that for a certain mass transfer rate, a certain amount of matter accumulates in the nearby regions of the system.

Type
VII. Related Objects
Information
International Astronomical Union Colloquium , Volume 93: Cataclysmic Variables: Recent Multi-Frequency Observations and Theoretical Developments , 1987 , pp. 675 - 679
Copyright
Copyright © Reidel 1987

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