On Evolution Of Contact Eclipsing Binaries

Details On Evolution Of Contact Eclipsing Binaries On Evolution Of Contact Eclipsing Binaries

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.246..309k&link_type=abstract

Astrophysics and Space Science, Volume 246, Issue 2, pp.309-314

Astronomy and Astrophysics

Astrophysics

Scientific paper

It is shown that during contact eclipsing binaries evolution under the influence of stellar wind, magnetic stellar wind and with matter transfer by gas flow, in binary stellar systems there may take place a process of star merger (low mass stars) within 105 107 yr and a fast increase of distance between stars of massive binaries. W UMa-type stars are a finite evolutionary stage of very close and low mass binary pairs. As for contact systems of early spectral types (CE-systems), they are more varied in evolution.

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