Volume 362 -
Multifrequency Behaviour of High Energy Cosmic Sources - XIII (MULTIF2019) -
Astrophysics of High Energy Cosmic Sources
Gamma-ray binaries
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Pre-published on:
November 23, 2020
Published on:
December 03, 2020
Abstract
Gamma-ray binaries are a subclass of high-mass binary systems whose energy spectrum peaks at high energies (HE, E>100 MeV) and extends to very high energies (VHE, E>100 GeV) gamma-rays. In this review we summarize properties of well-studied non-transient gamma-ray binaries as well as briefly discuss poorly known systems and transient systems hosting a microquasar. We also discuss theoretical models that have been used to describe spectral and timing characteristics of considered systems.
DOI: https://doi.org/10.22323/1.362.0045
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.