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arXiv · 2006.03615

Gamma-ray binaries

Maria Chernyakova·Denys Malyshev
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Abstract

Gamma-ray binaries are a subclass of high-mass binary systems whose energy spectrum peaks at high energies (E$\gtrsim$100 MeV) and extends to very high energies (E$\gtrsim$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 discuss also theoretical models that have been used to describe spectral and timing characteristics of considered systems

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Maria Chernyakova, Denys Malyshev. 2020-06-05. Gamma-ray binaries. https://arxiv.org/abs/2006.03615

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