Stochastic mass loss rate fluctuations and evolution of massive stars

Details Stochastic mass loss rate fluctuations and evolution of massive stars Stochastic mass loss rate fluctuations and evolution of massive stars

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..85...17n&link_type=abstract

Astrophysics and Space Science, vol. 85, no. 1-2, July 1982, p. 17-23. Research supported by the Consiglio Nazionale delle Rice

Astronomy and Astrophysics

Astrophysics

Stellar Evolution, Stellar Mass Ejection, Stellar Models, Stellar Winds, Stochastic Processes, Supermassive Stars, Chemical Composition, Hertzsprung-Russell Diagram, Supergiant Stars

Scientific paper

Stochastic fluctuations were superimposed on the rate of mass loss as determined according to the radiation-pressure stellar-wind theory to evaluate the effects on the evolution of a 60-solar masses star. If the variations in the rate are of the order of those observed, there are no significant modifications of the stellar parameters, and the agreement between theory and observations cannot be improved taking into account stochastic fluctuations.

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