{
  "id": "astro-ph/0405014",
  "version": "v1",
  "published": "2004-05-03T09:44:58.000Z",
  "updated": "2004-05-03T09:44:58.000Z",
  "title": "An Interpretation of the $hν_{peak}$ - $E_{iso}$ Correlation for GRB",
  "authors": [
    "David Eichler",
    "Amir Levinson"
  ],
  "comment": "12 pages. 5 figures",
  "journal": "Astrophys.J. 614 (2004) L13-L16",
  "doi": "10.1086/425310",
  "categories": [
    "astro-ph"
  ],
  "abstract": "The $h\\nu_{peak}/100 KeV \\sim [E_{iso}/10^{52} \\rm{erg}]^{1/2}$ correlation reported recently by Amati et al. (2002) and Lamb et al. (2003) for long GRB's can be interpreted as a viewing angle effect if the emitting region of the fireball is ring-shaped.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2004-05-03T09:44:58.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "correlation",
      "interpretation",
      "long grbs"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 12,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 649491
    }
  }
}