Basic relations between physical parameters of Wolf-Rayet stars

Details Basic relations between physical parameters of Wolf-Rayet stars Basic relations between physical parameters of Wolf-Rayet stars

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...263..129s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 263, no. 1-2, p. 129-136.

Astronomy and Astrophysics

Astrophysics

104

Stellar Models, Wolf-Rayet Stars, Abundance, Stellar Composition, Stellar Cores, Stellar Luminosity, Stellar Mass Ejection, Stellar Temperature

Scientific paper

Several simple relations are derived for WR stars between mass, luminosity, radius, surface temperature, and T(eff) obtained from new grids of stellar models by Schaller et al. (1992). Evolutionary models are described which predict a relation between the initial ZAMS mass and the luminosity of the WNL and WNE stars. Surface abundances of He, C, and O of WC/WO stars and their dependence on mass loss are reported.

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