{
  "id": "1003.5555",
  "version": "v1",
  "published": "2010-03-29T14:49:36.000Z",
  "updated": "2010-03-29T14:49:36.000Z",
  "title": "Implicit hydrodynamic simulations of stellar interiors",
  "authors": [
    "Maxime Viallet",
    "Isabelle Baraffe",
    "Cedric Mulet-Marquis",
    "Emmanuel Leveque",
    "Rolf Walder",
    "Bernd Freytag",
    "Christophe Winisdoerffer"
  ],
  "comment": "To appear in the Proceedings of Astronum 2009, 4th Int. Conf. on Numerical Modeling of Space Plasma Flows (refereed paper)",
  "categories": [
    "astro-ph.SR",
    "astro-ph.IM"
  ],
  "abstract": "We report on the development of an implicit multi-D hydrodynamic code for stellar evolution. We present two test-cases relevant for the first scientific goal of the code: the simulation of convection in pulsating stars. First results on a realistic stellar model are also presented.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2010-03-29T14:49:36.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "implicit hydrodynamic simulations",
      "stellar interiors",
      "implicit multi-d hydrodynamic code",
      "first scientific goal",
      "realistic stellar model"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 850229,
      "adsabs": "2010ASPC..429..167V"
    }
  }
}