Observational evidences for the dependence of WNE-star mass loss on metallicity

Details Observational evidences for the dependence of WNE-star mass loss on metallicity Observational evidences for the dependence of WNE-star mass loss on metallicity

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..353..203n&link_type=abstract

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

Computer Science

1

Scientific paper

We determined the mass-loss rates and luminosities of WN2 - WN5 stars in
the LMC and SMC by using the empirically scaled formulae. The comparison
of these mass-loss rates and luminosities with the respective data for
the Galactic WN stars allows to estimate that mass-loss rates of WNE
stars depend on Z in the power of about 1.5 - 2.

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