{
  "id": "1510.02217",
  "version": "v1",
  "published": "2015-10-08T07:53:36.000Z",
  "updated": "2015-10-08T07:53:36.000Z",
  "title": "Determining the evolutionary stage of HD163899 on the basis of its oscillation spectrum",
  "authors": [
    "Jakub Ostrowski",
    "Jadwiga Daszyńska-Daszkiewicz",
    "Henryk Cugier"
  ],
  "comment": "6 pages, 4 figures, conference",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We present the new interpretation of the oscillation spectrum of HD 163899 based on the new determinations of the effective temperature, mass-luminosity ratio and rotational velocity. These new parameters strongly prefer the more massive models than previously considered. Now it is also possible that the star could be in the main sequence stage. Using the oscillation spectrum as a gauge, we intend to establish which stage of evolution corresponds better to HD 163899.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2015-10-08T07:53:36.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "oscillation spectrum",
      "evolutionary stage",
      "evolution corresponds better",
      "main sequence stage",
      "mass-luminosity ratio"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 6,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "adsabs": "2015arXiv151002217O"
    }
  }
}