{
  "id": "1109.2373",
  "version": "v1",
  "published": "2011-09-12T03:38:58.000Z",
  "updated": "2011-09-12T03:38:58.000Z",
  "title": "A comparison of oscillation frequencies of rotating stars obtained by one- and two-dimensional calculations",
  "authors": [
    "Hideyuki Saio",
    "Robert G. Deupree"
  ],
  "comment": "4 pages, 3 figures; Proceedings of the 61st Fujihara Seminar: Progress in solar/stellar physics with helio- and asteroseismology, to appear in ASP Conference Series",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We discuss how the p- and g-mode frequencies calculated for rotating stars are affected by the way of including the centrifugal deformations. We find that p-mode frequencies are sensitive to the accuracy in treating the centrifugal deformation, while the effect becomes smaller for smaller frequencies in the g-mode range.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2011-09-12T03:38:58.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "rotating stars",
      "two-dimensional calculations",
      "oscillation frequencies",
      "comparison",
      "centrifugal deformation"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 927152,
      "adsabs": "2012ASPC..462..398S"
    }
  }
}