Calculation of the mass loss rate of binary systems through winds or expanding shells

Details Calculation of the mass loss rate of binary systems through winds or expanding shells Calculation of the mass loss rate of binary systems through winds or expanding shells

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996cha%26a..20q.508z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 20, Issue 4, p. 508-508.

Astronomy and Astrophysics

Astrophysics

Scientific paper

The P Cygni profiles of 22 Vul, AX Per and other ζ Aur systems are
calculated including multi-level transitions in hydrogen-helium mixtures
and assuming circular orbits. The derived rates of mass loss are
satisfactory.

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