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Rotational Angular Momenta of Close Binary System Components

Published online by Cambridge University Press:  14 August 2015

V. Ureche
V. Ureche*
Affiliation:
University of Cluj-Napoca, Cluj-Napoca, Roumania

Abstract

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The ratio between rotational angular momentum, J rot, and orbital angular momentum, J orb, in close binary systems and its variation with mass ratio is studied. The tables and the graphs give this variation for detached systems, contact systems, semidetached systems and for systems containing a supernova-remnant component and a contact component. For this study some statistical relations of close binary stars were used.

The ratio J rot/J orb is sensitive to the variation of the mass ratio q. If q differs much from unity and if the concentration of the stellar matter is moderate (polytropic index n ~ 3), the neglect of rotational angular momentum, J rot, is not justified.

Information

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 73: Structure and Evolution of Close Binary Systems , 1976 , pp. 351 - 363
Copyright
Copyright © Reidel 1976 

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