« Hadronic models for gamma-ray emitting microquasars » |
Gustavo Romero |
Microquasars are accreting binary systems with relativistic jets. The jets produce non-thermal emission which has been detected, in some cases, from radio to TeV energies. In this talk I shall address the problem of what is the radiative output of these objects if a significant fraction of the relativistic particles in the jets are hadrons. Implications for high-energy gamma-ray and neutrino astronomy will be brielfy discussed. |
vendredi 21 novembre 2008 - 11:00 Salle des séminaires Évry Schatzman, Institut d'Astrophysique de Paris |
Page web du séminaire / Seminar's webpage |