The structure of close binaries

Details The structure of close binaries The structure of close binaries

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..54..199r&link_type=abstract

Astrophysics and Space Science, vol. 54, no. 1, Mar. 1978, p. 199-209.

Astronomy and Astrophysics

Astrophysics

Binary Stars, Companion Stars, Heat Transfer, Stellar Models, Convective Heat Transfer, Mathematical Models, Radiative Heat Transfer, Stellar Rotation

Scientific paper

A method for calculating the structure of a close binary component is
presented. It is seen that the effect of binary distortion is to shift
the zero age main sequence to the right. Attempts to construct contact
systems with these models confirm the results of earlier workers that
this is not possible.

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