On the influence of clumping on O and Wolf-Rayet spectra
Overwhelming observational and theoretical evidence suggests that the winds of massive stars are highly clumped. We briefly discuss the influence of clumping on model diagnostics and the difficulties of allowing for the influence of clumping on model spectra. Because of its simplicity, and because o...
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| Format: | Others |
| Language: | English |
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Universität Potsdam
2007
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| Online Access: | http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-17903 http://opus.kobv.de/ubp/volltexte/2008/1790/ |