{
  "id": "1304.1956",
  "version": "v1",
  "published": "2013-04-07T04:46:38.000Z",
  "updated": "2013-04-07T04:46:38.000Z",
  "title": "Magnetic Fields and the Formation of Cores and Disks",
  "authors": [
    "Shantanu Basu",
    "Nicole D. Bailey",
    "Wolf B. Dapp"
  ],
  "comment": "8 pages, 6 figures, to appear in ASP Conference Series, New Trends in Radio Astronomy in the ALMA Era, ed. S. Yamamoto",
  "categories": [
    "astro-ph.SR",
    "astro-ph.GA"
  ],
  "abstract": "We review recent results of non-ideal magnetohydrodynamic models for the fragmentation of molecular clouds and the collapse of cloud cores to form protostar-disk systems. Thin-disk models can elucidate many aspects of the physical problem and allow the calculation of large dynamic range of time and length scales.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2013-04-07T04:46:38.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "magnetic fields",
      "large dynamic range",
      "non-ideal magnetohydrodynamic models",
      "form protostar-disk systems",
      "length scales"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 8,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1227438,
      "adsabs": "2013ASPC..476..103B"
    }
  }
}