The influence of clumping on predicted O star wind parameters
We study the influence of clumping on the predicted wind structure of O-type stars. For this purpose we artificially include clumping into our stationary wind models. When the clumps are assumed to be optically thin, the radiative line force increases compared to corresponding unclumped models, with...
| Main Authors: | , , |
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| Format: | Others |
| Language: | English |
| Published: |
Universität Potsdam
2007
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| Subjects: | |
| Online Access: | http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-17969 http://opus.kobv.de/ubp/volltexte/2008/1796/ |