Loss of orbital angular momentum in close binary systems during their evolution

Details Loss of orbital angular momentum in close binary systems during their evolution Loss of orbital angular momentum in close binary systems during their evolution

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..64..177c&link_type=abstract

Astrophysics and Space Science, vol. 64, no. 1, Aug. 1979, p. 177-182.

Astronomy and Astrophysics

Astrophysics

8

Angular Momentum, Binary Stars, Mass Transfer, Orbital Mechanics, Stellar Evolution, Regression Analysis, Stellar Mass, Stellar Mass Ejection, Stellar Motions, Tables (Data)

Scientific paper

A total 91 binary systems of systemic mass less than 6.5 M0 have been studied. It is found that binary systems obey the relation: log H = C - 1.8 log M where C is constant having values - 1.18, -2.12 and -2.27 respectively for detached, semi-detached and contact binary systems. It is inferred that during evolution, the systemic orbital angular momentum decreases

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