{
  "id": "1202.4581",
  "version": "v1",
  "published": "2012-02-21T10:07:59.000Z",
  "updated": "2012-02-21T10:07:59.000Z",
  "title": "Presupernova evolution and explosive nucleosynthesis of zero metal massive stars",
  "authors": [
    "M. Limongi",
    "A. Chieffi"
  ],
  "comment": "39 pages, 8 figures, 2 tables, accepted for publication in ApJS",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We present a new set of zero metallicity models in the range 13-80 $\\rm M_\\odot$ together to the associated explosive nucleosynthesis. These models are fully homogeneous with the solar metallicity set we published in Limongi & Chieffi (2006) and will be freely available at the web site http://www.iasf-roma.inaf.it./orfeo/public{\\_}html. A comparison between these yields and an average star that represents the average behavior of most of the very metal poor stars in the range $\\rm -5.0<[Fe/H]<-2.5$ confirms previous findings that only a fraction of the elemental [X/Fe] may be fitted by the ejecta of $\\it standard$ core collapse supernovae.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2012-02-21T10:07:59.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "zero metal massive stars",
      "explosive nucleosynthesis",
      "presupernova evolution",
      "solar metallicity set",
      "zero metallicity models"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1088/0067-0049/199/2/38",
      "journal": "The Astrophysical Journal Supplement Series",
      "year": 2012,
      "month": "Apr",
      "volume": 199,
      "number": 2,
      "pages": 38
    },
    "note": {
      "typesetting": "TeX",
      "pages": 39,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1089937,
      "adsabs": "2012ApJS..199...38L"
    }
  }
}