High-energy flares from jet-clump interactions
High-mass microquasars are binary systems composed by a massive star and a compact object from which relativistic jets are launched. Regarding the companion star, observational evidence supports the idea that winds of hot stars are formed by clumps. Then, these inhomogeneities may interact with the...
| 主要な著者: | , , |
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| フォーマット: | Journal article |
| 出版事項: |
Astronomical Society of the Pacific
2010
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