{
  "id": "2006.03615",
  "version": "v1",
  "published": "2020-06-05T18:10:19.000Z",
  "updated": "2020-06-05T18:10:19.000Z",
  "title": "Gamma-ray binaries",
  "authors": [
    "Maria Chernyakova",
    "Denys Malyshev"
  ],
  "comment": "Conference Proceedings: \"Multifrequency Behaviour of High Energy Cosmic Sources\" - XIII - MULTIF2019",
  "categories": [
    "astro-ph.HE"
  ],
  "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",
  "revisions": [
    {
      "version": "v1",
      "updated": "2020-06-05T18:10:19.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "gamma-ray binaries",
      "high energies",
      "energy spectrum peaks",
      "high-mass binary systems",
      "transient systems"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}