Mass Transfer in Close Binary Systems - Original and Remnant Masses

Details Mass Transfer in Close Binary Systems - Original and Remnant Masses Mass Transfer in Close Binary Systems - Original and Remnant Masses

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...125..388b&link_type=abstract

Astronomy and Astrophysics, Vol.125, NO. 2, P. 388, 1983

Astronomy and Astrophysics

Astrophysics

Scientific paper

The comparison of the masses of numerous Algol binaries (and a few Wolf-Rayet systems) with some new relevant theoretical predictions, in which the influence of overshooting in stellar interiors is considered, appears to reconfirm that usual mass transfer computations cannot satisfactorily account for the observed masses of the post-mass exchange (case B) remnants.

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