Leptonic emission from microquasar jets: from radio to very high-energy gamma-rays
Microquasars are sources of very high-energy gamma-rays and, very probably, highenergy gamma-ray emitters. We propose a model for a jet that can allow to give accurate observational predictions for jet emission at different energies and provide with physical information of the object using multiwave...
Guardado en:
| Autores principales: | Bosch Ramon, V., Paredes, J. M., Romero, Gustavo Esteban |
|---|---|
| Formato: | Articulo Comunicacion |
| Lenguaje: | Inglés |
| Publicado: |
2005
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/124871 |
| Aporte de: |
Ejemplares similares
-
Gamma-ray and neutrino emission from misaligned microquasars
por: Romero, Gustavo Esteban, et al.
Publicado: (2005) -
A broadband leptonic model for gamma-ray emitting microquasars
por: Bosch Ramon, V., et al.
Publicado: (2006) -
High-mass microquasars and low-latitude gamma-ray sources
por: Bosch Ramon, V., et al.
Publicado: (2005) -
A microquasar model applied to unidentified gamma-ray sources
por: Bosch-Ramon, V., et al.
Publicado: (2006) -
Gamma-ray emission from early-type stars interacting with AGN jets
por: Araudo, Anabella Teresa, et al.
Publicado: (2013)