{
  "id": "1310.1725",
  "version": "v1",
  "published": "2013-10-07T10:49:51.000Z",
  "updated": "2013-10-07T10:49:51.000Z",
  "title": "Magnetic fields along the pre-main-sequence phase",
  "authors": [
    "E. Alecian"
  ],
  "comment": "10 pages, 1 figure. To appear in the conference proceedings \"Putting A Stars into Context: Evolution, Environment, and Related Stars\" held in Moscow, 2013",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "In this contribution I review some of the major work that have been undertaken in the last decade to study the magnetic fields in intermediate-mass pre-main sequence stars, with the goal of understanding the origin of the magnetic fields detected in the chemically peculiar Ap/Bp stars, and testing the fossil field theory.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2013-10-07T10:49:51.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "magnetic fields",
      "pre-main-sequence phase",
      "intermediate-mass pre-main sequence stars",
      "chemically peculiar ap/bp stars",
      "fossil field theory"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 10,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "adsabs": "2014psce.conf...84A"
    }
  }
}