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The Physical Constraints on a New LoBAL QSO at z=4.82
Yi WM(易卫敏)1,2,3; Green, Richard4; Bai JM(白金明)1,2,3; Wang, Tinggui5; Grier, Catherine J.6; Trump, Jonathan R.6,7,8; Brandt, William N.6,8; Zuo, Wenwen9; Yang, Jinyi10; Wang, Feige10; Yang, Chenwei5; Wu, Xue-Bing10,11; Zhou, Hongyan12; Fan, Xiaohui4; Jiang, Linhua10,11; Yang, Qian10; Varricatt, Watson13; Kerr, Tom13; Milne, Peter4; Benigni, Sam13; Wang JG(王建国)1,2,3; Zhang JJ(张居甲)1,2,3; Wang F(王放)1,2; Wang CJ(王传军)1,2,14; Xin YX(辛玉新)1,2,14; Fan YF(范玉峰)1,2,3; Chang L(常亮)1,2,3; Zhang XL(张西亮)1,2,3; Lun BL(伦宝利)1,2,3; Yi, Weimin(Chinese Acad Sci, Yunnan Observ, Kunming 650216, Peoples R China)
发表期刊ASTROPHYSICAL JOURNAL
2017-04-01
卷号838期号:2
DOI10.3847/1538-4357/aa65d6
产权排序第1完成单位
收录类别SCI
关键词Galaxies: High-redshift Quasars: Absorption Lines Quasars: General Quasars: Individual (j0122+1216)
摘要Very few low-ionization broad absorption line (LoBAL) QSOs have been found at high redshifts, to date. One high-redshift LoBAL QSO, J0122+1216, was recently discovered by the Lijiang 2.4 m Telescope, with an initial redshift determination of 4.76. Aiming to investigate its physical properties, we carried out follow-up observations in the optical and near-IR spectroscopy. Near-IR spectra from UKIRT and P200 confirm that it is a LoBAL, with a new redshift determination of 4.82 +/- 0.01 based on the Mg II emission-line. The new Mg II redshift determination reveals strong blueshifts and asymmetry of the high-ionization emission lines. We estimate a black hole mass of similar to 2.3 x 10(9) M-circle dot and Eddington ratio of similar to 1.0 according to the empirical Mg II-based single-epoch relation and bolometric correction factor. It is possible that strong outflows are the result of an extreme quasar environment driven by the high Eddington ratio. A lower limit on the outflowing kinetic power (>0.9% L-Edd) is derived from both emission and absorption lines, indicating that these outflows play a significant role in the feedback process that regulates the growth of its black hole, as well as host galaxy evolution.
项目资助者West Light Foundation of The Chinese Academy of Sciences(Y6XB016001) ; China Scholarships Council(201604910001) ; NSF(AST-1516784, AST-1517113) ; Key Research Program of the CAS(KJZD-EW-M06) ; NSFC(11133006, 11433004) ; NASA ; National Astronomical Observatories of China ; Chinese Academy of Sciences (Strategic Priority Research Program "The Emergence of Cosmological Structures")(XDB09000000) ; Special Fund for Astronomy from the Ministry of Finance ; CAS ; People's Government of Yunnan Province
语种英语
学科领域天文学
文章类型Article
ISSN0004-637X
URL查看原文
WOS记录号WOS:000398296700011
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]BROAD-ABSORPTION-LINE ; DIGITAL-SKY-SURVEY ; ACTIVE GALACTIC NUCLEI ; BLACK-HOLE MASS ; QUASI-STELLAR OBJECTS ; EMISSION-LINE ; DATA RELEASE ; C-IV ; MULTIYEAR TIMESCALES ; DISTANT QUASARS
引用统计
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/10019
专题丽江天文观测站(南方基地)
中国科学院天体结构与演化重点实验室
通讯作者Yi, Weimin(Chinese Acad Sci, Yunnan Observ, Kunming 650216, Peoples R China)
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China
2.Center for Astronomical Mega-science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, P. R. China
3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, China
4.Steward Observatory, University of Arizona, Tucson, AZ 85721-0065, USA
5.CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, China
6.Department of Astronomy & Astrophysics and Institute for Gravitation & the Cosmos, The Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802, USA
7.Department of Physics, University of Connecticut, 2152 Hillside Road Unit 3046, Storrs, CT 06269, USA
8.Department of Physics, Pennsylvania State University, University Park, PA, 16802, USA
9.Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China
10.Department of Astronomy, School of Physics, Peking University, Beijing 100871, China
11.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China
12.Polar Research Institute of China, 451 Jinqiao Road, Shanghai 200136, China
13.UKIRT Observatory, Hilo, HI 96720, USA
14.University of the Chinese Academy of Sciences, Beijing 100049, China
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Yi WM,Green, Richard,Bai JM,et al. The Physical Constraints on a New LoBAL QSO at z=4.82[J]. ASTROPHYSICAL JOURNAL,2017,838(2).
APA Yi WM.,Green, Richard.,Bai JM.,Wang, Tinggui.,Grier, Catherine J..,...&Yi, Weimin.(2017).The Physical Constraints on a New LoBAL QSO at z=4.82.ASTROPHYSICAL JOURNAL,838(2).
MLA Yi WM,et al."The Physical Constraints on a New LoBAL QSO at z=4.82".ASTROPHYSICAL JOURNAL 838.2(2017).
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