{
  "id": "astro-ph/9709153",
  "version": "v1",
  "published": "1997-09-16T15:36:10.000Z",
  "updated": "1997-09-16T15:36:10.000Z",
  "title": "Nucleosynthesis in Classical Novae: ONe vs. CO White Dwarfs",
  "authors": [
    "Jordi Jose",
    "Margarita Hernanz"
  ],
  "comment": "38 pages, Latex file, with 3 ps figures. Accepted for publication in The Astrophysical Journal",
  "journal": "Astrophys.J.494:680-690,1998",
  "doi": "10.1086/305244",
  "categories": [
    "astro-ph"
  ],
  "abstract": "Detailed nucleosynthesis in the ejecta of classical novae has been determined for a grid of hydrodynamic nova models. The reported 14 evolutionary sequences, followed from the onset of accretion up to the explosion and ejection stages, span a range of CO and ONe white dwarf masses (0.8-1.35 $M_o$) and mixing levels between the accreted envelope and the underlying white dwarf core (25-75%). The synthesis of each isotope, from ${}^1$H to ${}^{40}$Ca, is discussed along with its sensitivity to model parameters. Special emphasis is given to isotopes such as ${}^{13}$C, ${}^{15}$N, and ${}^{17}$O, which may account for a significant fraction of their Galactic content. Production of the radioactive isotopes ${}^7$Be, ${}^{22}$Na, and ${}^{26}$Al is also analyzed, since they may provide a direct test of the thermonuclear runaway model through their $\\gamma$-ray emission. The resulting elemental yields reproduce fairly well the spectroscopic abundance determinations of several well studied classical novae.",
  "revisions": [
    {
      "version": "v1",
      "updated": "1997-09-16T15:36:10.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "classical novae",
      "elemental yields reproduce",
      "nucleosynthesis",
      "spectroscopic abundance determinations",
      "thermonuclear runaway model"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "LaTeX",
      "pages": 38,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 462125
    }
  }
}