{
  "id": "1109.1768",
  "version": "v1",
  "published": "2011-09-08T16:47:54.000Z",
  "updated": "2011-09-08T16:47:54.000Z",
  "title": "Uncertaities due to convection and production of s-nuclei in massive stars",
  "authors": [
    "M. L. Pumo",
    "G. Contino",
    "A. Bonanno",
    "R. A. Zappalà"
  ],
  "comment": "4 pages, no figures, Proceedings of the \"54{\\deg} congresso della Societa' Astronomica Italiana\", Napoli, May 4-7, 2010, to appear in Mem. S.A.It. Suppl",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We have investigated the role of the convective overshooting on the production of s-nuclei during core He-burning phase in stellar models with different initial mass and metallicity ($15 \\leq M_{ZAMS}/M_{\\odot} \\leq 25$; $10^{-4} \\leq Z \\leq 0.02$), considering a diffusive approach to model the convective overshooting. The results and their possible consequences on some open questions linked to the s-process weak component efficiency are discussed.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2011-09-08T16:47:54.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "massive stars",
      "production",
      "convection",
      "s-process weak component efficiency",
      "uncertaities"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 926859,
      "adsabs": "2012MSAIS..19..197P"
    }
  }
}