J. M. Paredes
Published 2006-09-06Version 1
I review here some of the main observational features in microquasars and AGNs as sources of high-energy gamma-rays as well as some of the current models that try to explain the emission in the gamma-ray domain.
Comments: 12 pages, 4 figures. Invited talk, to be published in the proceedings of the Vulcano Workshop 2006 "Frontier Objects in Astrophysics and Particle Physics", F. Giovannelli & G. Mannocchi (eds.), Italian Physical Society, Editrice Compositori, Bologna, Italy
High-energy gamma-ray Emission from Microquasars: LS 5039 and LS I +61 303
Introduction to Astrophysics of Microquasars
Phase-Resolved Studies of the High-Energy Gamma-Ray Emission from the Crab, Geminga, and Vela Pulsars
