High energy processes in microquasars
天体物理学
2009-11-10 v1
摘要
Microquasars are X-ray binary stars with the capability to generate relativisticjets. It is expected that microquasars are gamma-ray sources, because of the analogy with quasars and because the theoretical models predict emission at such energy range. In addition, from observational arguments, there are two microquasars that appear as the possible counterparts for two unidentified high-energy gamma-ray sources.
引用
@article{arxiv.astro-ph/0501576,
title = {High energy processes in microquasars},
author = {Josep M. Paredes},
journal= {arXiv preprint arXiv:astro-ph/0501576},
year = {2009}
}
备注
Universitat de Barcelona, Departament d'Astronomia i Meteorologia, 12 pages, 5 figures. Invited talk presented at the International Symposium "High-Energy Gamma-Ray Astronomy", 26-30 July 2004, Heidelberg (Germany). To be published by AIP Proceedings Series