The Mass Ratio Distribution of Close Binary Stars with the Components Belonging to Main Sequence

Details The Mass Ratio Distribution of Close Binary Stars with the Components Belonging to Main Sequence The Mass Ratio Distribution of Close Binary Stars with the Components Belonging to Main Sequence

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988atsir1527...19k&link_type=abstract

Astronomicheskii Tsirkulyar NO.1527/MAR-A, P. 19, 1988

Astronomy and Astrophysics

Astronomy

Scientific paper

Contemporary and initial mass ratio distributions of detached close
binaries with both components belonging to the main sequence are
investigated. They seem to be unimodal, with a single maximum near q =
1. The dependence of q as a function of mass of the main component is
revealed.

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