Mass-luminosity relation for Wolf-Rayet stars

Details Mass-luminosity relation for Wolf-Rayet stars Mass-luminosity relation for Wolf-Rayet stars

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...262..483b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 262, no. 2, p. 483-486.

Astronomy and Astrophysics

Astrophysics

5

Mass To Light Ratios, Stellar Luminosity, Wolf-Rayet Stars, Power Series, Stellar Structure

Scientific paper

A mass-luminosity relation for Wolf-Rayet (WR) stars based on the mass-luminosity relation of the standard model and the Eddington quartic is presented. It is shown that this mass-luminosity law explains well the recent calculations of Langer (1989). The hypothesis that the observable properties of WR stars (except WNL) depend only on their mass and surface chemical composition is discussed.

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