Expected gamma-ray emission from x-ray binaries
High Energy Astrophysical Phenomena
2015-06-03 v1
Abstract
It is at present well known that conditions at some massive binary systems allow acceleration of particles and production of the GeV-TeV gamma-rays. However, which particles are responsible for this emission and what radiation processes are engaged is at present not completely clear. We discuss what parameters can determine the acceleration process of particles and high energy radiation produced by them within massive binary systems.
Keywords
Cite
@article{arxiv.1111.5904,
title = {Expected gamma-ray emission from x-ray binaries},
author = {W. Bednarek},
journal= {arXiv preprint arXiv:1111.5904},
year = {2015}
}
Comments
12 pages, 6 figures, in Proc. HEPRO III Conference (eds. J.M. Paredes & M. Ribo), accepted to Int.J.Mod.Phys.Conf.Series