Wind relics : clumps, inhomogeneities and outflows in LBV nebulae
The most massive stars are those with the shortest but most active life. One group of massive stars, the Luminous Blue Variables (LBVs), of which only a few objects are known, are in particular of interest concerning the stability of stars. They have a high mass loss rate and are close to being inst...
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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-18235 http://opus.kobv.de/ubp/volltexte/2008/1823/ |