Non-thermal processes around accreting galactic black holes
Context. Accreting black holes in galactic X-ray sources are surrounded by hot plasma. The innermost part of these systems is likely a corona with different temperatures for ions and electrons. In the so-called low-hard state, hot electrons Comptonize soft X-ray photons from the disk that partially...
Guardado en:
| Autores principales: | Romero, Gustavo Esteban, Vieyro, Florencia Laura, Vila, Gabriela Soledad |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2010
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/82513 |
| Aporte de: |
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