Using gamma-rays to probe the clumped structure of stellar winds
Gamma-rays can be produced by the interaction of a relativistic jet and the matter of the stellar wind in the subclass of massive X-ray binaries known as "microquasars". The relativistic jet is ejected from the surroundings of the compact object and interacts with cold protons from the ste...
| Main Authors: | , , , , |
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| Format: | Conference item |
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Universitätsverlag Potsdam
2008
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