{
  "id": "astro-ph/0611594",
  "version": "v1",
  "published": "2006-11-18T13:28:09.000Z",
  "updated": "2006-11-18T13:28:09.000Z",
  "title": "Modeling of the Super-Eddington Phase for Classical Novae: Five IUE Novae",
  "authors": [
    "Mariko Kato",
    "Izumi Hachisu"
  ],
  "comment": "9 pages including 8 figures, to appear in the Astrophysical Journal",
  "journal": "Astrophys.J.657:1004-1012,2007",
  "doi": "10.1086/511058",
  "categories": [
    "astro-ph"
  ],
  "abstract": "We present a light curve model for the super-Eddington luminosity phase of five classical novae observed with IUE. Optical and UV light curves are calculated based on the optically thick wind theory with a reduced effective opacity for a porous atmosphere. Fitting a model light curve with the UV 1455 \\AA light curve, we determine the white dwarf mass and distance to be (1.3 M_sun, 4.4 kpc) for V693 CrA, (1.05 M_sun, 1.8 kpc) for V1974 Cyg, (0.95 M_sun, 4.1 kpc) for V1668 Cyg, (1.0 M_sun, 2.1 kpc) for V351 Pup, and (1.0 M_sun, 4.3 kpc) for OS And.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2006-11-18T13:28:09.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "classical novae",
      "iue novae",
      "super-eddington phase",
      "light curve model",
      "white dwarf mass"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 9,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 732185
    }
  }
}