High-energy emission from accreting black holes with high-mass donor stars
We present an analysis of the interactions of a distribution of relativistic protons under the typical conditions of the corona surrounding an accreting black hole. The model is applied to a concrete binary system with a high-mass donor star: the classical source Cygnus X-1
Guardado en:
| Autores principales: | , |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2008
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/97510 https://ri.conicet.gov.ar/11336/22920 http://adsabs.harvard.edu/abs/2008RMxAC..33..122V http://www.astroscu.unam.mx/rmaa/RMxAC..33/PDF/RMxAC..33_gvila.pdf |
| Aporte de: |
| Sumario: | We present an analysis of the interactions of a distribution of relativistic protons under the typical conditions of the corona surrounding an accreting black hole. The model is applied to a concrete binary system with a high-mass donor star: the classical source Cygnus X-1 |
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