Constraints on wind clumping from the empirical mass-loss vs. metallicity relation for early-type stars
We present the latest results on the observational dependence of the mass-loss rate in stellar winds of O and early-B stars on the metal content of their atmospheres, and compare these with predictions. Absolute empirical rates for the mass loss of stars brighter than 10$^{5.2} L_{odot}$, based on H...
| 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-17736 http://opus.kobv.de/ubp/volltexte/2008/1773/ |