Wolf-Rayet stars of the carbon sequence

A. Barniske, W.-R. Hamann, G. Gräfener

Universität Potsdam, Institut für Physik, Astrophysik

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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