{
  "id": "1805.05963",
  "version": "v1",
  "published": "2018-05-15T18:00:10.000Z",
  "updated": "2018-05-15T18:00:10.000Z",
  "title": "HD 63021: An Ae Star with X-ray Flux",
  "authors": [
    "David G. Whelan",
    "Jon Labadie-Bartz",
    "S. Drew Chojnowski",
    "James Daglen",
    "Ken Hudson"
  ],
  "comment": "4 pages, 1 figure. Accepted for publication in RNAAS, Number 2, 2018",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "Balmer and Fe II (42) multiplet emission were discovered in a spectrum of HD 63021 on 10 April (UTC), 2018. Subsequent observations revealed variability in both photospheric absorption lines and Balmer line emission. In addition, it is an X-ray source, with a luminosity that is consistent with either a very strong stellar wind, or else the presence of a compact binary companion. Spectroscopic and photometric followup are planned to determine the nature of this source.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2018-05-15T18:00:10.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "x-ray flux",
      "ae star",
      "strong stellar wind",
      "subsequent observations revealed variability",
      "photospheric absorption lines"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}