{
  "id": "0901.3319",
  "version": "v1",
  "published": "2009-01-21T17:16:25.000Z",
  "updated": "2009-01-21T17:16:25.000Z",
  "title": "New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars",
  "authors": [
    "S. Hubrig",
    "M. Briquet",
    "P. De Cat",
    "M. Schoeller",
    "T. Morel",
    "I. Ilyin"
  ],
  "comment": "2 pages, 1 figure, to appear in Proceedings of IAU Symposium 259 \"Cosmic Magnetic Fields: from Planets, to Stars and Galaxies\", Tenerife, Spain, November 3-7, 2008",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We present the results of the continuation of our magnetic survey with FORS1 at the VLT of a sample of B-type stars consisting of confirmed or candidate beta Cephei stars and Slowly Pulsating B stars. Roughly one third of the studied beta Cephei stars have detected magnetic fields. The fraction of magnetic Slowly Pulsating B and candidate Slowly Pulsating B stars is found to be higher, up to 50%. We find that the domains of magnetic and non-magnetic pulsating stars in the H-R diagram largely overlap, and no clear picture emerges as to the possible evolution of the magnetic field across the main sequence.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2009-01-21T17:16:25.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "magnetic field measurements",
      "slowly pulsating",
      "candidate beta cephei stars",
      "h-r diagram largely overlap",
      "clear picture emerges"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 2,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 811627
    }
  }
}