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Paper: Wolf-Rayet stars of the carbon sequence
Volume: 353, Stellar Evolution at Low Metallicity: Mass Loss, Explosions, Cosmology
Page: 243
Authors: Barniske, A.; Hamann, W.-R.; Graefener, G.
Abstract: 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 WC5–8.
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