出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：High energy emission could be produced in the interaction sites of both galactic and extragalactic jets with the surrounding medium. We have developed an interaction model that accounts for the continuous injection of relativistic electrons in the forward, reverse and recollimation shocks. We also performed hydrodynamical simulations to establish the physical properties in both type of systems. The resulting non-thermal emission is predicted assuming different values for the jet power, the external mass density and the source age for both FR-I galaxies and galactic microquasars. The obtained fluxes are compared to current instrument sensitivities at radio, X-ray and gamma-ray bands. We study in detail the connection between hard X-ray synchrotron radiation and gamma-ray emission and use the INTEGRAL, Fermi and AGILE, and Cherenkov telescopes capabilities to test it.
