{
  "id": "1008.0561",
  "version": "v1",
  "published": "2010-08-03T14:50:11.000Z",
  "updated": "2010-08-03T14:50:11.000Z",
  "title": "Spectral energy distribution of gamma-ray binaries: Sources and Processes",
  "authors": [
    "V. Bosch-Ramon"
  ],
  "comment": "8 pages, 11 figures; invited talk at the conference \"Steady Jets and Transient Jets, Characteristics and Relationship\", held in Bonn, Germany, 7-8 April 2010, to be published in Memorie della Societa Astronomica Italiana",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "Gamma-ray binaries are suitable sources to study high-energy processes in jets and outflows in general. In the last years, there has been a lot of activity in the field of gamma-ray binaries to identify the different factors that shape their non-thermal spectra, which ranges from radio to very high energies, as well as their lightcurves. In this work, I discuss the main aspects of the non-thermal emission in this class of objects, which presently includes high-mass microquasars, high-mass binaries hosting a non-accreting pulsar and, probably, massive star binaries; few potential candidates to be gamma-ray binaries are also presented. Finally, the importance of gamma-ray absorption is discussed, and the main physical ingredients, which are likely involved in the non-thermal radiation in gamma-ray binaries, are briefly considered.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2010-08-03T14:50:11.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "gamma-ray binaries",
      "spectral energy distribution",
      "study high-energy processes",
      "high energies",
      "gamma-ray absorption"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 8,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 864229,
      "adsabs": "2011MmSAI..82..182B"
    }
  }
}