{
  "id": "astro-ph/0508570",
  "version": "v1",
  "published": "2005-08-26T03:32:56.000Z",
  "updated": "2005-08-26T03:32:56.000Z",
  "title": "The blueshift of the [O III] emission line in NLS1s",
  "authors": [
    "W. Bian",
    "Q. Yuan",
    "Y. Zhao"
  ],
  "comment": "11 Pages, 4 figures, 3 tales, accepted for publication in MNRAS",
  "categories": [
    "astro-ph"
  ],
  "abstract": "We investigate the radial velocity difference between the narrow emission-line components of [O III] $\\lambda$ 5007 and H$\\beta$ in a sample of 150 SDSS NLS1s. Seven \"blue outliers\" with [O III] blueshifted by more than 250 \\kms are found. A strong correlation between the [O III] blueshift and the Eddington ratio is found for these seven \"blue outliers\". For the entire sample, we found a modest correlation between the blueshift and the linewidth of the narrow component of the [O III] line. The reflected profile of [O III] indicates two kinematically and physically distinct regions. The [O III] linewidth depends not only on the bulge stellar gravitational potential, but also on the central black hole potential.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2005-08-26T03:32:56.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "emission line",
      "central black hole potential",
      "blue outliers",
      "bulge stellar gravitational potential",
      "radial velocity difference"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 11,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 690829,
      "adsabs": "2005astro.ph..8570B"
    }
  }
}