NAOC Open IR
Eddington-limited Accretion in z similar to 2 WISE-selected Hot, Dust-obscured Galaxies
Wu, Jingwen1,2; Jun, Hyunsung D.3,4; Assef, Roberto J.5; Tsai, Chao-Wei2; Wright, Edward L.2; Eisenhardt, Peter R. M.3; Blain, Andrew6; Stern, Daniel3; Diaz-Santos, Tanio5; Denney, Kelly D.7,8; Hayden, Brian T.9,10; Perlmutter, Saul9,10; Aldering, Greg9; Boone, Kyle9,10; Fagrelius, Parker9,10
2018-01-10
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume852Issue:2Pages:15
AbstractHot, dust-obscured galaxies, or "Hot DOGs," are a rare, dusty, hyperluminous galaxy population discovered by the WISE mission. Predominantly at redshifts 2-3, they include the most luminous known galaxies in the universe. Their high luminosities likely come from accretion onto highly obscured supermassive black holes (SMBHs). We have conducted a pilot survey to measure the SMBH masses of five z similar to 2 Hot DOGs via broad Ha emission lines, using Keck/MOSFIRE and Gemini/FLAMINGOS-2. We detect broad H alpha emission in all five Hot DOGs. We find substantial corresponding SMBH masses for these Hot DOGs (similar to 10(9) M-circle dot), and their derived Eddington ratios are close to unity. These z similar to 2 Hot DOGs are the most luminous active galactic nuclei for their BH masses, suggesting that they are accreting at the maximum rates for their BHs. A similar property is found for known z similar to 6 quasars. Our results are consistent with scenarios in which Hot DOGs represent a transitional, high-accretion phase between obscured and unobscured quasars. Hot DOGs may mark a special evolutionary stage before the red quasar and optical quasar phases, and they may be present at other cosmic epochs.
Keywordgalaxies: evolution galaxies: high-redshift galaxies: ISM infrared: galaxies quasars: supermassive black holes
Funding OrganizationNational 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 ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Research Foundation of Korea (NRF) - Ministry of Education ; FONDECYT ; FONDECYT ; ALMA-CONICYT ; ALMA-CONICYT ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; W. M. Keck Foundation ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NASA ; NASA ; 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 ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Research Foundation of Korea (NRF) - Ministry of Education ; FONDECYT ; FONDECYT ; ALMA-CONICYT ; ALMA-CONICYT ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; W. M. Keck Foundation ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NASA ; NASA ; 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 ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Research Foundation of Korea (NRF) - Ministry of Education ; FONDECYT ; FONDECYT ; ALMA-CONICYT ; ALMA-CONICYT ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; W. M. Keck Foundation ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NASA ; NASA ; 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 ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Research Foundation of Korea (NRF) - Ministry of Education ; FONDECYT ; FONDECYT ; ALMA-CONICYT ; ALMA-CONICYT ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; W. M. Keck Foundation ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NASA ; NASA
DOI10.3847/1538-4357/aa9ff3
WOS KeywordACTIVE GALACTIC NUCLEI ; BLACK-HOLE MASSES ; DIGITAL SKY SURVEY ; RADIUS-LUMINOSITY RELATIONSHIP ; EXTREMELY RED QUASARS ; IONIZED-GAS NEBULAE ; 7TH DATA RELEASE ; LINE-OF-SIGHT ; X-RAY SOURCE ; EMISSION-LINE
Language英语
Funding ProjectNational Key Program for Science and Technology Research and Development of China[2016YFA0400702] ; NSFC[11673029] ; National Research Foundation of Korea (NRF) - Ministry of Education[NRF-2017R1A6A3A04005158] ; FONDECYT[1151408] ; FONDECYT[1151239] ; ALMA-CONICYT[31130005] ; National Aeronautics and Space Administration[13-ADAP13-0092] ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; NASA
Funding OrganizationNational 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 ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Research Foundation of Korea (NRF) - Ministry of Education ; FONDECYT ; FONDECYT ; ALMA-CONICYT ; ALMA-CONICYT ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; W. M. Keck Foundation ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NASA ; NASA ; 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 ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Research Foundation of Korea (NRF) - Ministry of Education ; FONDECYT ; FONDECYT ; ALMA-CONICYT ; ALMA-CONICYT ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; W. M. Keck Foundation ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NASA ; NASA ; 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 ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Research Foundation of Korea (NRF) - Ministry of Education ; FONDECYT ; FONDECYT ; ALMA-CONICYT ; ALMA-CONICYT ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; W. M. Keck Foundation ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NASA ; NASA ; 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 ; National Research Foundation of Korea (NRF) - Ministry of Education ; National Research Foundation of Korea (NRF) - Ministry of Education ; FONDECYT ; FONDECYT ; ALMA-CONICYT ; ALMA-CONICYT ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; W. M. Keck Foundation ; W. M. Keck Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NASA ; NASA
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000422716100003
PublisherIOP PUBLISHING LTD
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/37375
Collection中国科学院国家天文台
Corresponding AuthorWu, Jingwen
Affiliation1.Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China
2.Univ Calif Los Angeles, 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, 85 Hoegiro, Seoul 02455, South Korea
5.Univ Diego Portales, Av Republ 180, Santiago, Region Metropol, Chile
6.Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
7.Ohio State Univ, Dept Astron, 140 West 18th Ave, Columbus, OH 43210 USA
8.Illuminat Works LLC, 5550 Blazer Pkwy, Dublin, OH 43017 USA
9.EO Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
10.Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
Recommended Citation
GB/T 7714
Wu, Jingwen,Jun, Hyunsung D.,Assef, Roberto J.,et al. Eddington-limited Accretion in z similar to 2 WISE-selected Hot, Dust-obscured Galaxies[J]. ASTROPHYSICAL JOURNAL,2018,852(2):15.
APA Wu, Jingwen.,Jun, Hyunsung D..,Assef, Roberto J..,Tsai, Chao-Wei.,Wright, Edward L..,...&Fagrelius, Parker.(2018).Eddington-limited Accretion in z similar to 2 WISE-selected Hot, Dust-obscured Galaxies.ASTROPHYSICAL JOURNAL,852(2),15.
MLA Wu, Jingwen,et al."Eddington-limited Accretion in z similar to 2 WISE-selected Hot, Dust-obscured Galaxies".ASTROPHYSICAL JOURNAL 852.2(2018):15.
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