PARTICLE ACCELERATION IN THE COLLIDING WIND BINARY WR 140
Massive WR+O star systems produce high-temperature, shock-heated plasma where the wind of the WR star and that of its binary companion collide ¿ the wind-collision region (WCR). The WCR is a source of thermal (e.g. hard X-rays) and non-thermal (e.g. synchrotron) emission, the latter arising from ele...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2008
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57116159027 |
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