Variability and theoretical upper limit of the mass loss rate in OB-stars

Details Variability and theoretical upper limit of the mass loss rate in OB-stars Variability and theoretical upper limit of the mass loss rate in OB-stars

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...94..109v&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 94, no. 1, July 1992, p. 109-120.

Statistics

Computation

11

B Stars, O Stars, Stellar Mass Ejection, Stellar Winds, Variability, Computational Astrophysics, Line Spectra, Stellar Models

Scientific paper

Solutions of the stellar wind equations for 70 O-type and 19 B-type individual stars are presented. The calculated mass loss rates M, terminal velocities v(infinity) and line profiles are compared with the observed ones. It is shown that a theoretical upper limit of the mass loss rate exists. Wind variability in connection with this critical mass loss rate is discussed.

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