Coupling hydrodynamics and radiation calculations for star-jet interactions in AGN
Stellar populations can contribute to the non-thermal emission of radio-loud active galactic nuclei via the interaction with the relativistic jets. The shock produced between the stellar wind and the jet can accelerate particles and produce high-energy emission. We have performed 2D axisymmetric hyd...
Guardado en:
| Autores principales: | de la Cita, Víctor, Bosch-Ramon, Valentí, Paredes Fortuny, Xavier, Khangulyan, Dmitry, Perucho, Manel |
|---|---|
| Formato: | Objeto de conferencia |
| Lenguaje: | Inglés |
| Publicado: |
2015
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/167853 |
| Aporte de: |
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