{
  "id": "1401.4761",
  "version": "v1",
  "published": "2014-01-20T00:22:39.000Z",
  "updated": "2014-01-20T00:22:39.000Z",
  "title": "Simulations of Accretion onto Magnetized Stars: Results of 3D MHD Simulations and 3D Radiative Transfer",
  "authors": [
    "Marina Romanova",
    "Ryuichi Kurosawa"
  ],
  "comment": "6 pages, 5 figures, to appear in the proceedings of ASTRONUM-2013 meeting: \"8th International Conference on Numerical Modeling of Space Plasma Flows\", Biarritz, France, July 1-5, 2013",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We discuss the results of modelling of young magnetized stars, where matter flow is calculated using the three-dimensional (3D) magneto-hydrodynamic (MHD) \"Cubed Sphere\" code, and the spectra are calculated using the 3D Monte Carlo radiative transfer code \"TORUS\". Two examples of modelling are shown: (1) accretion onto stars in stable and unstable regimes, and (2) accretion to a young star V2129 Oph, modelled with realistic parameters.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2014-01-20T00:22:39.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "3d mhd simulations",
      "3d radiative transfer",
      "magnetized stars",
      "monte carlo radiative transfer code",
      "3d monte carlo radiative transfer"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 6,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "adsabs": "2014ASPC..488..127R"
    }
  }
}