A unified formula for mass-loss rate of O to M stars

Details A unified formula for mass-loss rate of O to M stars A unified formula for mass-loss rate of O to M stars

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...331..932t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 331, Aug. 15, 1988, p. 932-938.

Statistics

Computation

11

Computational Astrophysics, Conservation Equations, M Stars, O Stars, Stellar Mass Ejection, Stellar Winds, B Stars, Radiation Pressure, Stellar Luminosity, Stellar Spectra

Scientific paper

A formula for stellar mass-loss rate has been derived using conservation equations of mass and momentum for coronal and continuum radiation-driven wind. The derived mass-loss rate formula has been found to be consistent with the observed mass-loss rates for stars from O to M spectral type. Two constant parameters appearing in the mass-loss rate formula have been found to have values for special group of stars such as Be-stars, which are different from the majority of stars.

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