{
  "id": "0907.0976",
  "version": "v1",
  "published": "2009-07-06T12:49:49.000Z",
  "updated": "2009-07-06T12:49:49.000Z",
  "title": "Predicted gamma-ray image of SN 1006 due to inverse Compton emission",
  "authors": [
    "O. Petruk",
    "F. Bocchino",
    "M. Miceli",
    "G. Dubner",
    "G. Castelletti",
    "S. Orlando",
    "D. Iakubovskyi",
    "I. Telezhinsky"
  ],
  "comment": "10 pages, 11 figures, accepted in MNRAS",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "We propose a method to synthesize the inverse Compton (IC) gamma-ray image of a supernova remnant starting from the radio (or hard X-ray) map and using results of the spatially resolved X-ray spectral analysis. The method is successfully applied to SN 1006. We found that synthesized IC gamma-ray images of SN 1006 show morphology in nice agreement with that reported by the H.E.S.S. collaboration. The good correlation found between the observed very-high energy gamma-ray and X-ray/radio appearance can be considered as an evidence that the gamma-ray emission of SN 1006 observed by H.E.S.S. is leptonic in origin, though the hadronic origin may not be excluded.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2009-07-06T12:49:49.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "inverse compton emission",
      "predicted gamma-ray image",
      "spatially resolved x-ray spectral analysis",
      "very-high energy gamma-ray",
      "synthesized ic gamma-ray images"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1111/j.1365-2966.2009.15352.x",
      "journal": "Monthly Notices of the Royal Astronomical Society",
      "year": 2009,
      "month": "Oct",
      "volume": 399,
      "number": 1,
      "pages": 157
    },
    "note": {
      "typesetting": "TeX",
      "pages": 10,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 825021,
      "adsabs": "2009MNRAS.399..157P"
    }
  }
}