{
  "id": "1012.2357",
  "version": "v1",
  "published": "2010-12-10T19:22:17.000Z",
  "updated": "2010-12-10T19:22:17.000Z",
  "title": "An analysis of the magnetic field geometry and its interaction with the circumstellar environment of HD 57682 by the MiMeS Collaboration",
  "authors": [
    "J. H. Grunhut",
    "G. A. Wade",
    "W. L. F. Marcolino",
    "V. Petit",
    "H. F. Henrichs",
    "the MiMeS Collaboration"
  ],
  "comment": "3 pages, 3 figures, to appear in the proceedings of Magnetic Stars 2010",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We will review our recent analysis of the magnetic properties of the O9IV star HD 57682, using spectropolarimetric observations obtained with ESPaDOnS at the Canada-France-Hawaii telescope within the context of the Magnetism in Massive Stars (MiMeS) Large Program. We discuss our most recent determination of the rotational period from longitudinal magnetic field measurements and H_alpha variability - the latter obtained from over a decade's worth of professional and amateur spectroscopic observations. Lastly, we report on our investigation of the magnetic field geometry and the effects of the field on the circumstellar environment.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2010-12-10T19:22:17.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "magnetic field geometry",
      "circumstellar environment",
      "mimes collaboration",
      "interaction",
      "longitudinal magnetic field measurements"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 3,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 880860,
      "adsabs": "2011mast.conf..473G"
    }
  }
}