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Super-Eddington Accretion in the WISE-selected Extremely Luminous Infrared Galaxy W2246-0526

文献类型：期刊论文

作者Tsai, Chao-Wei2; Eisenhardt, Peter R. M.3; Jun, Hyunsung D.4; Wu, Jingwen5; Assef, Roberto J.6; Blain, Andrew W.7; Diaz-Santos, Tanio6; Jones, Suzy F.1; Stern, Daniel3; Wright, Edward L.2
刊名ASTROPHYSICAL JOURNAL
出版日期2018-11-20
卷号868期号:1页码:9
关键词infrared: galaxies galaxies: active galaxies: individual (WISEA J224607.56-052634.9) galaxies: nuclei quasars: emission lines quasars: supermassive black holes
ISSN号0004-637X
DOI10.3847/1538-4357/aae698
英文摘要We use optical and near-infrared spectroscopy to observe rest-UV emission lines and estimate the black hole mass of WISEA J224607.56-052634.9 (W2246-0526) at z = 4.601, the most luminous hot, dust-obscured galaxy yet discovered by WISE. From the broad component of the Mg II 2799 A emission line, we measure a black hole mass of log(M-BH/M-circle dot)= 9.6 +/- 0.4. The broad C IV 1549 A line is asymmetric and significantly blueshifted. The derived M-BH from the blueshift-corrected broad C IV line width agrees with the Mg II result. From direct measurement using a well-sampled SED, the bolometric luminosity is 3.6 x 10(14) L-circle dot. The corresponding Eddington ratio for W2246-0526 is lambda(Edd) = L-AGN/L-Edd = 2.8. This high Eddington ratio may reach the level where the luminosity is saturating due to photon trapping in the accretion flow and may be insensitive to the mass accretion rate. In this case, the MBH growth rate in W2246-0526. would exceed the apparent accretion rate derived from the observed luminosity.
WOS关键词ACTIVE GALACTIC NUCLEI ; BLACK-HOLE MASSES ; SPECTRAL ENERGY-DISTRIBUTIONS ; SIMILAR-TO 2 ; EMISSION-LINE ; HIGH-REDSHIFT ; INTERSTELLAR-MEDIUM ; TYPE-1 QUASARS ; MG II ; ULTRAVIOLET
资助项目National Aeronautics and Space Administration through the Astrophysics Data Analysis Program[13-ADAP13-0092] ; National Research Foundation of Korea (NRF) - Ministry of Education[NRF-2017R1A6A3A04005158] ; National Key Program for Science and Technology Research and Development of China[2016YFA0400702] ; NSFC[11673029] ; FONDECYT[1151408] ; ALMA-CONICYT[31130005] ; FONDECYT regular project[1151239] ; W.M. Keck Foundation ; National Aeronautics and Space Administration
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000450221800015
出版者IOP PUBLISHING LTD
资助机构National Aeronautics and Space Administration through the Astrophysics Data Analysis Program ; National Aeronautics and Space Administration through the Astrophysics Data Analysis Program ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Key Program for Science and Technology Research and Development of China ; National Key Program for Science and Technology Research and Development of China ; NSFC ; NSFC ; FONDECYT ; FONDECYT ; ALMA-CONICYT ; ALMA-CONICYT ; FONDECYT regular project ; FONDECYT regular project ; W.M. Keck Foundation ; W.M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration through the Astrophysics Data Analysis Program ; National Aeronautics and Space Administration through the Astrophysics Data Analysis Program ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Key Program for Science and Technology Research and Development of China ; National Key Program for Science and Technology Research and Development of China ; NSFC ; NSFC ; FONDECYT ; FONDECYT ; ALMA-CONICYT ; ALMA-CONICYT ; FONDECYT regular project ; FONDECYT regular project ; W.M. Keck Foundation ; W.M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration through the Astrophysics Data Analysis Program ; National Aeronautics and Space Administration through the Astrophysics Data Analysis Program ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Key Program for Science and Technology Research and Development of China ; National Key Program for Science and Technology Research and Development of China ; NSFC ; NSFC ; FONDECYT ; FONDECYT ; ALMA-CONICYT ; ALMA-CONICYT ; FONDECYT regular project ; FONDECYT regular project ; W.M. Keck Foundation ; W.M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration through the Astrophysics Data Analysis Program ; National Aeronautics and Space Administration through the Astrophysics Data Analysis Program ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Key Program for Science and Technology Research and Development of China ; National Key Program for Science and Technology Research and Development of China ; NSFC ; NSFC ; FONDECYT ; FONDECYT ; ALMA-CONICYT ; ALMA-CONICYT ; FONDECYT regular project ; FONDECYT regular project ; W.M. Keck Foundation ; W.M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration
源URL[http://ir.bao.ac.cn/handle/114a11/23372]  
专题中国科学院国家天文台
通讯作者Tsai, Chao-Wei
作者单位1.Chalmers Univ Technol, Onsala Space Observ, Dept Space Earth & Environm, Onsala, Sweden
2.UCLA, Dept Phys & Astron, Los Angeles, CA 90095 USA
3.CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
4.Korea Inst Adv Study, Sch Phys, Seoul 02455, South Korea
5.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
6.Univ Diego Portales, Nucleo Astron, Fac Ingn & Ciencias, Ave Ejercito Libertador 441, Santiago, Chile
7.Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
8.WM Keck Observ, Kamuela, HI 96743 USA
推荐引用方式
GB/T 7714		 Tsai, Chao-Wei,Eisenhardt, Peter R. M.,Jun, Hyunsung D.,et al. Super-Eddington Accretion in the WISE-selected Extremely Luminous Infrared Galaxy W2246-0526[J]. ASTROPHYSICAL JOURNAL,2018,868(1):9.
APA Tsai, Chao-Wei.,Eisenhardt, Peter R. M..,Jun, Hyunsung D..,Wu, Jingwen.,Assef, Roberto J..,...&Yeh, Sherry C. C..(2018).Super-Eddington Accretion in the WISE-selected Extremely Luminous Infrared Galaxy W2246-0526.ASTROPHYSICAL JOURNAL,868(1),9.
MLA Tsai, Chao-Wei,et al."Super-Eddington Accretion in the WISE-selected Extremely Luminous Infrared Galaxy W2246-0526".ASTROPHYSICAL JOURNAL 868.1(2018):9.

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来源：国家天文台

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