{
  "id": "1603.02397",
  "version": "v1",
  "published": "2016-03-08T06:52:17.000Z",
  "updated": "2016-03-08T06:52:17.000Z",
  "title": "SDSS J163459.82+204936.0: A Ringed Infrared-Luminous Quasar with Outflows in both Absorption and Emission Lines",
  "authors": [
    "Wen-Juan Liu",
    "Hong-Yan Zhou",
    "Ning Jiang",
    "Xufen Wu",
    "Jianwei Lyu",
    "Xiheng Shi",
    "Xinwen Shu",
    "Peng Jiang",
    "Tuo Ji",
    "Jiang-Guo Wang",
    "Shu-Fen Wang",
    "Luming Sun"
  ],
  "comment": "13 figures, 6 tables; Submitted to ApJ",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "SDSS J1634+2049 is a local (z = 0.1293) infrared-luminous quasar with LIR= 10^11.91 Lsun. We present a detailed multiwavelength study of both the host galaxy and the nucleus. The host galaxy demonstrates violent, obscured star formation activities with SFR ~ 140 Msun yr^-1, estimated from either the PAH emission or IR luminosity. The optical to NIR spectra exhibit a blueshifted narrow cuspy component in Hb, HeI5876,10830 and other emission lines consistently with an offset velocity of ~900 km/s, as well as additional blueshifting phenomena in high-ionization lines , while there exist blueshifted broad absorption lines (BALs) in NaID and HeI*3889,10830, indicative of the AGN outflows producing BALs and emission lines. Constrained mutually by the several BALs with CLOUDY, the physical properties of the absorption-line outflow are derived as follows: 10^4 < n_H <= 10^5 cm^-3, 10^-1.3 <= U <= 10^-0.7 and 10^22.5<= N_H <= 10^22.9 cm^-2 , similar to those derived for the emission-line outflows. The similarity suggests a common origin. Taking advantages of both the absorption lines and outflowing emission lines, we find that the outflow gas is located at a distance of 48 - 65 pc from the nucleus, and that the kinetic luminosity of the outflow is 10^44-10^46 erg s^-1. J1634+2049 has a off-centered galactic ring on the scale of ~ 30 kpc that is proved to be formed by a recent head-on collision by a nearby galaxy. Thus this quasar is a valuable object in the transitional phase emerging out of dust enshrouding as depicted by the co-evolution scenario.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2016-03-08T06:52:17.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "emission lines",
      "ringed infrared-luminous quasar",
      "host galaxy demonstrates violent",
      "blueshifted narrow cuspy component",
      "blueshifted broad absorption lines"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}