Comparison of remnant masses from close binary evolution with estimates derived from new single star models

Details Comparison of remnant masses from close binary evolution with estimates derived from new single star models Comparison of remnant masses from close binary evolution with estimates derived from new single star models

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...277..475d&link_type=abstract

Astronomy and Astrophysics, Vol. 277, p. 475 (1993)

Astronomy and Astrophysics

Astrophysics

1

Stars: Evolution Binaries - Close - Stars: Interiors

Scientific paper

Recent models of single stars with updated input physics are compared to
binary models. The comparison shows that the remnant masses after mass
transfer from the latter calculations are comparable to those that can
be expected from the new models.

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