{
  "id": "1401.5374",
  "version": "v1",
  "published": "2014-01-21T16:30:13.000Z",
  "updated": "2014-01-21T16:30:13.000Z",
  "title": "Formation and appearance of pulsar-like white dwarfs",
  "authors": [
    "Nazar Ikhsanov",
    "Nina Beskrovnaya"
  ],
  "comment": "3 pages, to appear in Proc. of Thirteenth Marcel Grossmann Meeting - MG13",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "Accretion-driven spin-up of a magnetized white dwarf in a close binary system is discussed. We address a situation in which the magnetic field of the white dwarf is screening during the accretion phase and re-generating due to the field diffusion through the accreted material after it. We find this scenario to be effective for a formation of massive pulsar-like white dwarfs.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2014-01-21T16:30:13.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "appearance",
      "close binary system",
      "magnetized white dwarf",
      "massive pulsar-like white dwarfs",
      "field diffusion"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1142/9789814623995_0467"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 3,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1278323,
      "adsabs": "2015mgm..conf.2453I"
    }
  }
}