{
  "id": "0902.0528",
  "version": "v2",
  "published": "2009-02-03T15:19:06.000Z",
  "updated": "2009-02-10T18:02:55.000Z",
  "title": "Star-powered LINERs in the Sloan Digital Sky Survey",
  "authors": [
    "N. Vale Asari",
    "G. Stasinska",
    "R. Cid Fernandes",
    "J. M. Gomes",
    "M. Schlickmann",
    "A. Mateus",
    "W. Schoenell",
    "L. Sodre Jr.",
    "for the SEAGal collaboration"
  ],
  "comment": "To appear in the proceedings of \"The Starburst-AGN Connection\" conference (2008). Corrected Fig. 3",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "Galaxies are usually classified as star forming or active by using diagnostic diagrams, such as [N II]/Halpha vs. [O III]/Hbeta. Active galaxies are further classified into Seyfert or LINER-like sources. We claim that a non-negligible fraction of galaxies classified as LINERs in the Sloan Digital Sky Survey are in fact ionized by hot post-AGB stars and white dwarfs.",
  "revisions": [
    {
      "version": "v2",
      "updated": "2009-02-10T18:02:55.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "sloan digital sky survey",
      "star-powered liners",
      "hot post-agb stars",
      "diagnostic diagrams",
      "white dwarfs"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 812454,
      "adsabs": "2009arXiv0902.0528V"
    }
  }
}