{
  "id": "1002.1379",
  "version": "v1",
  "published": "2010-02-06T12:45:49.000Z",
  "updated": "2010-02-06T12:45:49.000Z",
  "title": "X-Ray and Gamma-Ray Emission from the Galactic Center",
  "authors": [
    "V. A. Dogiel",
    "K. -S. Cheng",
    "D. O. Chernyshov",
    "W. -H. Ip",
    "C. -M. Ko",
    "V. Tatischeff"
  ],
  "comment": "5 pages, Contributed talk for the proceedings of the Galactic Center Workshop 2009, \"The Galactic Center: A Window to the Nuclear Environment of Disk Galaxies\", in 19-21 October, Shanghai China, 19-21 October, 2009",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "We discuss the origin of continuum and line X-ray emission observed in the direction the Galactic Center. We predict a significant flux of de-excitation gamma-ray lines in this direction, which can be produced by subrelativistic protons generated by accretion processes.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2010-02-06T12:45:49.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "galactic center",
      "gamma-ray emission",
      "line x-ray emission",
      "de-excitation gamma-ray lines",
      "significant flux"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 5,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 845056,
      "adsabs": "2011ASPC..439..426D"
    }
  }
}