Evolution in semi-detached binary systems

Details Evolution in semi-detached binary systems Evolution in semi-detached binary systems

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..73..503c&link_type=abstract

Astrophysics and Space Science, vol. 73, no. 2, Dec. 1980, p. 503-506.

Astronomy and Astrophysics

Astrophysics

2

Angular Momentum, Eclipsing Binary Stars, Stellar Evolution, Stellar Motions, B Stars, Mass Ratios, Roche Limit, Stellar Mass

Scientific paper

The evolutionary process of semidetached binary systems is considered on the basis of nonconservation of orbital angular momentum. Initial periods for 54 Algol-type binaries are calculated using relations given by Chaubey (1979) and assuming an initial mass ratio of 1.2 (the average mass ratio for unevolved binaries). It is found that the semidetached binary systems follow Type B evolution.

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