Wolf-Rayet stars of the carbon sequence

Details Wolf-Rayet stars of the carbon sequence Wolf-Rayet stars of the carbon sequence

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..353..243b&link_type=abstract

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

Physics

6

Scientific paper

We established a grid of model atmospheres for WC stars with the Potsdam
Wolf-Rayet (PoWR) code. Clumping and iron line blanketing are taken into
account. The models are employed to analyze Galactic WC stars with
subtypes WC 5--8.

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