Lepto-hadronic model for the broadband emission of Cygnus X-1
Context. Cygnus X-1 is a well-observed microquasar. Broadband observations at all wavelengths have been collected over the years. The origin of the MeV tail observed with COMPTEL and INTEGRAL is still under debate and it has mostly been attributed to the corona, although its high degree of polarizat...
Guardado en:
| Autores principales: | Pepe, Carolina, Vila, Gabriela Soledad, Romero, Gustavo Esteban |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2015
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/86334 |
| Aporte de: |
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