{ "id": "1409.1580", "version": "v1", "published": "2014-09-04T20:00:13.000Z", "updated": "2014-09-04T20:00:13.000Z", "title": "A Census of Gas Outflows in Type 2 Active Galactic Nuclei", "authors": [ "Hyun-Jin Bae", "Jong-Hak Woo" ], "comment": "12 pages, 10 figures; Accepted to ApJ", "categories": [ "astro-ph.GA" ], "abstract": "We perform a census of ionized gas outflows using a sample of ~23,000 type 2 active galactic nuclei (AGNs) out to z~0.1. By measuring the velocity offset of narrow emission lines, i.e., [O III] {\\lambda}5007 and H{\\alpha}, with respect to the systemic velocity measured from the stellar absorption lines, we find that 47% of AGNs display an [O III] line-of-sight velocity offset $\\geq$ 20 km/s. The fraction of the [O III] velocity offset in type 2 AGNs is comparable to that in type 1 AGNs after considering the projection effect. AGNs with a large [O III] velocity offset preferentially have a high Eddington ratio, implying that the detected velocity offsets are related to black hole activity. The distribution of the host galaxy inclination is clearly different between the AGNs with blueshifted [O III] and the AGNs with redshifted [O III], supporting the combined model of the biconical outflow and dust obscuration. In addition, for ~3% of AGNs, [O III] and H{\\alpha} show comparable large velocity offsets, indicating a more complex gas kinematics than decelerating outflows in a stratified narrow-line region.", "revisions": [ { "version": "v1", "updated": "2014-09-04T20:00:13.000Z" } ], "analyses": { "keywords": [ "active galactic nuclei", "gas outflows", "narrow emission lines", "comparable large velocity offsets", "line-of-sight velocity offset" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/795/1/30", "journal": "The Astrophysical Journal", "year": 2014, "month": "Nov", "volume": 795, "number": 1, "pages": 30 }, "note": { "typesetting": "TeX", "pages": 12, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2014ApJ...795...30B" } } }