High energy emission from microquasars
Astrophysics
2015-06-24 v1
Abstract
The microquasar phenomenon is associated with the production of jets by X-ray binaries and, as such, may be associated with the majority of such systems. In this chapter we briefly outline the associations, definite, probable, possible, and speculative, between such jets and X-ray, gamma-ray and particle emission.
Cite
@article{arxiv.astro-ph/0310538,
title = {High energy emission from microquasars},
author = {Rob Fender and Tom Maccarone},
journal= {arXiv preprint arXiv:astro-ph/0310538},
year = {2015}
}
Comments
Contributing chapter to the book Cosmic Gamma-Ray Sources, K.S. Cheng and G.E. Romero (eds.), to be published by Kluwer Academic Publishers, Dordrecht, 2004. (19 pages)