Evolutionary effects in the stellar mass ratios of close binary systems

Details Evolutionary effects in the stellar mass ratios of close binary systems Evolutionary effects in the stellar mass ratios of close binary systems

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998arep...42..476k&link_type=abstract

Astronomy Reports, Volume 42, Issue 4, July 1998, pp.476-484

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The correlation between the stellar mass ratio q for eclipsing binary systems and the masses M_1 and M_2 of the stars is investigated. Contact and semi-detached systems display reliable correlations between the mass ratio q and the mass of the secondary M_2. For both classes of binaries studied, the rate with which q decreases as M_2 decreases becomes slower for more massive stars.

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