{
  "id": "1103.3070",
  "version": "v1",
  "published": "2011-03-16T00:01:29.000Z",
  "updated": "2011-03-16T00:01:29.000Z",
  "title": "Spectroscopy of BL Cam - Observations",
  "authors": [
    "M. Alvarez",
    "R. Michel",
    "L. Fox-Machado",
    "J. P. Sareyan",
    "S. Fauvaud",
    "G. Tovmassian"
  ],
  "comment": "1 page, 1 figure, to appear in proceedings of XIII Latin American Regional IAU Meeting, Morelia-Michoacan, Mexico 2010, RevMexAA(SC)",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "The star BL Camelopardalis (GD 428, GSC 04067-00471, V=12.92, B=13.1), is a SX Phoenicis pulsating variable showing a high amplitude variability (300-350 mmag), with a very clear period of 56.3 min, that has being recently studied by Fauvaud et al. (2010). They show that the observed variability is due to a clear and single pulsation, as expected for these type of pulsators. It was discovered as a variable star on 1976 by Berg and Duthie (1977).",
  "revisions": [
    {
      "version": "v1",
      "updated": "2011-03-16T00:01:29.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "spectroscopy",
      "observations",
      "phoenicis pulsating variable showing",
      "star bl camelopardalis",
      "high amplitude variability"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 1,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 892838,
      "adsabs": "2011RMxAC..40..266A"
    }
  }
}