{
  "id": "1708.06757",
  "version": "v1",
  "published": "2017-08-22T08:35:11.000Z",
  "updated": "2017-08-22T08:35:11.000Z",
  "title": "Impact of NLTE on determinations of atmospheric parameters and chemical abundances of very metal-poor stars",
  "authors": [
    "Lyudmila Mashonkina",
    "Tatyana Sitnova",
    "Yuri Pakhomov",
    "Tatyana Ryabchikova"
  ],
  "comment": "Two pages, to appear in Rediscovering our Galaxy, Proceedings IAU Symposium No. 334, 2017, C. Chiappini, I. Minchev, E. Starkenburg & M. Valentini, eds",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "Based on high-resolution spectral observations for a sample of very metal-poor stars, we investigate how well stellar chemical abundances can be derived with available theoretical methods and computational tools.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2017-08-22T08:35:11.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "metal-poor stars",
      "atmospheric parameters",
      "determinations",
      "high-resolution spectral observations",
      "computational tools"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}