Optically thick wind models of WNE stars: the dependence of mass loss on metallicity

Details Optically thick wind models of WNE stars: the dependence of mass loss on metallicity Optically thick wind models of WNE stars: the dependence of mass loss on metallicity

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..353..191n&link_type=abstract

Stellar Evolution at Low Metallicity: Mass Loss, Explosions, Cosmology ASP Conference Series, Vol. 353, Proceedings of the Confe

Physics

1

Scientific paper

The dependence of mass-loss rates of WNE stars on metallicity Z has been
derived from the solutions of optically thick wind models. It appears
that the mass-loss rates of these stars depend quite strongly on Z
(dot{M} ∝ Z^{α} with α being equal to about 0.5 - 1 for
Z ≈ 0.002-0.02).

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