Journal
ASTRONOMY & ASTROPHYSICS
Volume 387, Issue 1, Pages 244-257Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20020269
Keywords
stars : Wolf-Rayet; stars : atmospheres; stars : abundances; stars : early-type; stars : mass loss; stars : individual : WR111
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We describe the treatment of iron group line-blanketing in non-LTE model atmospheres for WR stars. As an example, a blanketed model for the early-type WC star WR111 is compared to its un-blanketed counterpart. Blanketing affects the ionization structure and the emergent flux distribution of our models. The radiation pressure, as computed within our models, falls short by only a factor of two to provide the mechanical power of the WR wind.
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