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 multiwavelength data.
Información general
Fecha de publicación:2005
Idioma del documento:Inglés
Revista:Proceedings of the International Astronomical Union; vol. 1, no. S230
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