Clumping effects on non-thermal particle spectra in massive star systems
Observational evidence exists that winds of massive stars are clumped. Many massive star systems are known as non-thermal particle production sites, as indicated by their synchrotron emission in the radio band. As a consequence they are also considered as candidate sites for non-thermal high-energy...
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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-18246 http://opus.kobv.de/ubp/volltexte/2008/1824/ |