A universal formula for determining the stellar mass loss rate

Details A universal formula for determining the stellar mass loss rate A universal formula for determining the stellar mass loss rate

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15...42n&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Jan. 1989, p. 42-47. In Russian. In Russian. In Russian.

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Stellar Mass Ejection, Stellar Winds, Wolf-Rayet Stars, Computational Astrophysics, Iue, Stellar Luminosity

Scientific paper

The quiet outflow of stellar mass, which occurs as stellar wind, is
considered. Mass loss rates (M) for 400 stars were used to derive a
formula expressing M as a function of four stellar parameters: L,
T(eff), Y, and Z.

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