Gamma-ray binaries
High Energy Astrophysical Phenomena
2020-06-09 v1
Abstract
Gamma-ray binaries are a subclass of high-mass binary systems whose energy spectrum peaks at high energies (E100 MeV) and extends to very high energies (E100 GeV) rays. In this review we summarize properties of well-studied non-transient -ray binaries as well as briefly discuss poorly known systems and transient systems hosting a microquasar. We discuss also theoretical models that have been used to describe spectral and timing characteristics of considered systems
Cite
@article{arxiv.2006.03615,
title = {Gamma-ray binaries},
author = {Maria Chernyakova and Denys Malyshev},
journal= {arXiv preprint arXiv:2006.03615},
year = {2020}
}
Comments
Conference Proceedings: "Multifrequency Behaviour of High Energy Cosmic Sources" - XIII - MULTIF2019