Is the stellar system WR11 a gamma-ray source?
Many early-type stars are in systems; some of them have been indicated as putative high-energy emitters. The radiationwould be produced at the region where two stellar winds collide. Compelling evidence of such emission was found only for the colliding-wind binary (CWB) Eta Car, which was associated...
Guardado en:
| Autor principal: | Benaglia, Paula |
|---|---|
| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2016
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/102078 https://ri.conicet.gov.ar/11336/24341 http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=10294057&fulltextType=RA&fileId=S132335801600014X |
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