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SDSS J163459.82+204936.0: A RINGED INFRARED-LUMINOUS QUASAR WITH OUTFLOWS IN BOTH ABSORPTION AND EMISSION LINES
Liu WJ(刘文娟)1,2,3,4; Zhou, Hong-Yan1,4; Jiang, Ning4; Wu, Xufen4; Lyu, Jianwei5; Shi, Xiheng1; Shu, Xinwen6; Jiang, Peng1,7,8; Ji, Tuo1; Wang JG(王建国)2,3; Wang, Shu-Fen1,2,3; Sun, Luming1,4
Source PublicationASTROPHYSICAL JOURNAL
2016-05-10
Volume822Issue:2
DOI10.3847/0004-637X/822/2/64
Contribution Rank第2完成单位
Indexed BySCI
KeywordGalaxies: Active Galaxies: Individual (Sdss j163459.82+204936.0) Galaxies: Starburst Quasars: Absorption Lines Quasars: Emission Lines
Abstract

SDSS J163459.82+204936.0 is a local (z = 0.1293) infrared-luminous quasar with L-IR = 10(11.91) L-circle dot. We present a detailed multiwavelength study of both the host galaxy and the nucleus. The host galaxy, appearing as an early-type galaxy in the optical images and spectra, demonstrates violent, obscured star formation activities with SFR approximate to 140 M-circle dot yr(-1), estimated from either the polycyclic aromatic hydrocarbon emission or IR luminosity. The optical to NIR spectra exhibit a blueshifted narrow cuspy component in H beta, He I lambda lambda 5876, 10830, and other emission lines consistently with an offset velocity of approximate to 900 km s(-1), as well as additional blueshifting phenomena in high-ionization lines (e.g., a blueshifted broad component of He I lambda 10830 and the bulk blueshifting of [O III].5007), while there exist blueshifted broad absorption lines (BALs) in Na I. D and He I lambda lambda 3889, 10830, indicative of the active galactic nucleus outflows producing BALs and emission lines. Constrained mutually by the several BALs in the photoionization simulations with Cloudy, the physical properties of the absorption line outflow are derived as follows: density 10(4) < n(H) less than or similar to 10(5) cm(-3), ionization parameter 10(-1.3) less than or similar to U 10(-0.7), and column density 10(22.5) less than or similar to N-H less than or similar to 10(22.9) cm(-2), which are similar to those derived for the emission line outflows. This 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 similar to 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 similar to 30. kpc that is proved to be formed by a recent head-on collision by a nearby galaxy for which we spectroscopically measure the redshift. Thus, this quasar is a valuable object in the transitional phase emerging out of dust enshrouding as depicted by the coevolution scenario invoking galaxy merger (or violent interaction) and quasar feedback. Its proximity enables our further observational investigations in detail (or tests) of the co-evolution paradigm.

Funding ProjectSOC program[CHINARE2012-02-03] ; Natural Science Foundation of China[NSFC 11473025] ; Natural Science Foundation of China[11033007] ; Natural Science Foundation of China[11421303] ; Natural Science Foundation of China[NSFC 11203021] ; Natural Science Foundation of China[11573024] ; Natural Science Foundation of China[NSFC 11503025] ; Natural Science Foundation of China[NSFC 11573001] ; Natural Science Foundation of China[NSFC 11233002] ; Natural Science Foundation of China[NSFC 11303085] ; National Basic Research Program of China (the 973 Program)[2013CB834905] ; Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences[OP201408] ; Fundamental Research Funds for the Central Universities ; CAS ; People's Government of Yunnan Province ; Strategic Priority Research Program, "The Emergence of Cosmological Structures"[XDB09000000] ; National Astronomical Observatories ; Chinese Academy of Sciences ; Ministry of Finance
Funding OrganizationSOC program[CHINARE2012-02-03] ; Natural Science Foundation of China[NSFC 11473025, 11033007, 11421303, NSFC 11203021, 11573024, NSFC 11503025, NSFC 11573001, NSFC 11233002, NSFC 11303085] ; National Basic Research Program of China (the 973 Program)[2013CB834905] ; Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences[OP201408] ; Fundamental Research Funds for the Central Universities ; CAS ; People's Government of Yunnan Province ; Strategic Priority Research Program, "The Emergence of Cosmological Structures"[XDB09000000] ; National Astronomical Observatories ; Chinese Academy of Sciences ; Ministry of Finance
Language英语
Subject Area天文学 ; 星系与宇宙学
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherIOP PUBLISHING LTD
Publication PlaceTEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS IDWOS:000377204900007
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordACTIVE GALACTIC NUCLEI ; DIGITAL SKY SURVEY ; SPECTRAL ENERGY-DISTRIBUTIONS ; SUPERMASSIVE BLACK-HOLES ; SPITZER-SPACE-TELESCOPE ; LARGE-MAGELLANIC-CLOUD ; PALOMAR-GREEN QUASARS ; SEYFERT-1 GALAXIES ; INTERSTELLAR DUST ; ULIRG EVOLUTION
Citation statistics
Cited Times:6[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/9607
Collection自由探索组
中国科学院天体结构与演化重点实验室
Corresponding AuthorZhou, Hong-Yan
Affiliation1.Polar Research Institute of China, 451 Jinqiao Road, Shanghai 200136, China
2.Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan 650011, China
3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, Yunnan 650011, China
4.Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Sciences and Technology of China, Hefei, Anhui 230026, China
5.Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA
6.Department of Physics, Anhui Normal University, Wuhu, Anhui 241000, China
7.School of Astronomy and Space Science, Nanjing University, 22 Hankou Road, Nanjing 210093, China
8.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210093, China
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Liu WJ,Zhou, Hong-Yan,Jiang, Ning,et al. SDSS J163459.82+204936.0: A RINGED INFRARED-LUMINOUS QUASAR WITH OUTFLOWS IN BOTH ABSORPTION AND EMISSION LINES[J]. ASTROPHYSICAL JOURNAL,2016,822(2).
APA Liu WJ.,Zhou, Hong-Yan.,Jiang, Ning.,Wu, Xufen.,Lyu, Jianwei.,...&Sun, Luming.(2016).SDSS J163459.82+204936.0: A RINGED INFRARED-LUMINOUS QUASAR WITH OUTFLOWS IN BOTH ABSORPTION AND EMISSION LINES.ASTROPHYSICAL JOURNAL,822(2).
MLA Liu WJ,et al."SDSS J163459.82+204936.0: A RINGED INFRARED-LUMINOUS QUASAR WITH OUTFLOWS IN BOTH ABSORPTION AND EMISSION LINES".ASTROPHYSICAL JOURNAL 822.2(2016).
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