Relation Between the Degree of Filling up the Roche Lobe and the Properties of Eclipsing Binary Stars

Details Relation Between the Degree of Filling up the Roche Lobe and the Properties of Eclipsing Binary Stars Relation Between the Degree of Filling up the Roche Lobe and the Properties of Eclipsing Binary Stars

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988atsir1528...11k&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1528/MAY, P. 11, 1988

Astronomy and Astrophysics

Astronomy

Scientific paper

It is shown that stars of lower mass in main sequence systems (<5
M_sun;) fill up their Roche lobes less than by 50% whereas more massive
stars fill them up more than by 50%.

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