{
  "id": "1301.2499",
  "version": "v1",
  "published": "2013-01-11T13:56:57.000Z",
  "updated": "2013-01-11T13:56:57.000Z",
  "title": "2D non-perturbative modeling of oscillations in rapidly rotating stars",
  "authors": [
    "R-M. Ouazzani",
    "M-A. Dupret",
    "M. J. Goupil",
    "D. R. Reese"
  ],
  "comment": "4 pages, 1 figure, proceedings of the 4th HELAS International Conference, Lanzarote feb 2010, Astronomical Notes, 2010, 331, P 45",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We present and discuss results of a recently developped two dimensional non-perturbative method to compute accurate adiabatic oscillation modes of rapidly rotating stars . The 2D calculations fully take into account the centrifugal distorsion of the star while the non-perturbative method includes the full influence of the Coriolis acceleration. These characteristics allows us to compute oscillation modes of rapid rotators - from high order p-modes in $\\delta$Scuti stars, to low order p- and g-modes in $\\beta$ Cephei or Be stars.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2013-01-11T13:56:57.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "rapidly rotating stars",
      "2d non-perturbative modeling",
      "accurate adiabatic oscillation modes",
      "high order p-modes",
      "coriolis acceleration"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1210403
    }
  }
}