{
  "id": "1507.08443",
  "version": "v1",
  "published": "2015-07-30T10:44:50.000Z",
  "updated": "2015-07-30T10:44:50.000Z",
  "title": "Disk tracing for B[e] supergiants in the Magellanic Clouds",
  "authors": [
    "G. Maravelias",
    "M. Kraus",
    "A. Aret"
  ],
  "comment": "2 pages; 1 figure; submitted to the proceedings of the Physics of Evolved Stars - A conference dedicated to the memory of Olivier Chesneau, Nice, France, June 8-12, 2015",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "B[e] supergiants are evolved massive stars with a complex circumstellar environment. A number of important emission features probe the structure and the kinematics of the circumstellar material. In our survey of Magellanic Cloud B[e] supergiants we focus on the [OI] and [CaII] emission lines, which we identified in four more objects.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2015-07-30T10:44:50.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "magellanic cloud",
      "supergiants",
      "disk tracing",
      "important emission features probe",
      "complex circumstellar environment"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 2,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "adsabs": "2015EAS....71..229M"
    }
  }
}