{
  "id": "0905.3075",
  "version": "v1",
  "published": "2009-05-19T12:05:39.000Z",
  "updated": "2009-05-19T12:05:39.000Z",
  "title": "Line and Continuum Emission from the Galactic Center. III. Origin of 6.4 keV Line Emission from Molecular Clouds in the Galactic Center",
  "authors": [
    "Vladimir Dogiel",
    "Kwong-Sang Cheng",
    "Dmitrii Chernyshov",
    "Aya Bamba",
    "Atsushi Ichimura",
    "Hajime Inoue",
    "Chung-Ming Ko",
    "Motohide Kokubun",
    "Yoshitomo Maeda",
    "Kazuhisa Mitsuda",
    "Noriko Y. Yamasaki"
  ],
  "comment": "Accepted in PASJ, to be published in PASJ Vol.61 No.5, 2009",
  "categories": [
    "astro-ph.HE",
    "astro-ph.GA"
  ],
  "abstract": "We analyze the 6.4 keV line and continuum emission from the molecular cloud Sgr B2 and the source HESS J1745-303, which is supposed to be a complex of molecular gas. From the HESS results it follows that Sgr A is a source of high energy protons, which penetrate into molecular clouds producing there a TeV gamma-ray flux. We present arguments that Sgr A may also produce a flux of subrelativistic protons which generate the 6.4 keV line and bremsstrahlung continuum emission from the clouds.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2009-05-19T12:05:39.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "galactic center",
      "kev line emission",
      "molecular cloud sgr b2",
      "tev gamma-ray flux",
      "bremsstrahlung continuum emission"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 820835,
      "adsabs": "2009arXiv0905.3075D"
    }
  }
}