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astro-ph2005
The metallicity dependence of WR wind models
G. Gräfener, W. -R. Hamann
With the advance of stellar atmosphere modelling during the last few years, large progress in the understanding of Wolf-Rayet (WR) mass loss has been achieved. In the present paper…
astro-ph2004
Hydrodynamic model atmospheres for WR stars: Self-consistent modeling of a WC star wind
G. Gräfener, W. -R. Hamann
We present the first non-LTE atmosphere models for WR stars that incorporate a self-consistent solution of the hydrodynamic equations. The models account for iron-group line-blanke…