{
  "id": "astro-ph/0207639",
  "version": "v1",
  "published": "2002-07-29T22:40:16.000Z",
  "updated": "2002-07-29T22:40:16.000Z",
  "title": "Classical Novae as Super-Eddington Objects",
  "authors": [
    "Nir J. Shaviv"
  ],
  "comment": "6 pages, 7 figures, to appear in the proceedings of the International Conference on Classical Nova Explosions, Sitges, Spain, 20-24 May 2002",
  "journal": "AIP Conf.Proc. 637 (2003) 259-265",
  "doi": "10.1063/1.1518210",
  "categories": [
    "astro-ph"
  ],
  "abstract": "Several of the inconsistencies plaguing the field of novae are resolved once we consider novae to be steady state super-Eddington objects. In particular, we show that the super-Eddington shell burning state is a natural consequence of the equations of stellar structure, and that the predicted mass loss in the super-Eddington state agrees with nova observations. We also find that the transition phase of novae can be naturally explained as \"stagnating\" winds.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2002-07-29T22:40:16.000Z"
    }
  ],
  "analyses": {
    "subjects": [
      "97.30.Qt",
      "97.10.Xq",
      "97.10.Cv",
      "97.10.Me"
    ],
    "keywords": [
      "classical novae",
      "steady state super-eddington objects",
      "super-eddington shell burning state",
      "super-eddington state agrees",
      "natural consequence"
    ],
    "tags": [
      "conference paper",
      "journal article"
    ],
    "publication": {
      "publisher": "AIP",
      "journal": "AIP Conf. Proc."
    },
    "note": {
      "typesetting": "TeX",
      "pages": 6,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 591575,
      "adsabs": "2002AIPC..637..259S"
    }
  }
}