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The Role of the Most Luminous Obscured AGNs in Galaxy Assembly at z similar to 2

文献类型:期刊论文

作者Blain, Andrew7; Tsai, Chao-Wei3; Petty, Sara8; Farrah, Duncan13; Connolly, Brian1; Jones, Suzy10; Benford, Dominic11; Eisenhardt, Peter4; Bridge, Carrie4; Jarrett, Tom2
刊名ASTROPHYSICAL JOURNAL
出版日期2017-08-01
卷号844期号:2
关键词Galaxies: Evolution Galaxies: High-redshift Galaxies: Starburst Quasars: General
DOI10.3847/1538-4357/aa78f2
文献子类Article
英文摘要We present Hubble Space Telescope WFC3 F160W imaging and infrared spectral energy distributions for 12 extremely luminous, obscured active galactic nuclei (AGNs) at 1.8 < z < 2.7. selected via "hot, dust-obscured" mid-infrared colors. Their infrared luminosities span (2-15) x 10(13) L-circle dot, making them among the most luminous objects in the universe at z similar to 2. In all cases, the infrared emission is consistent with arising at least for the. most part from AGN activity. The AGN fractional luminosities are higher than those in either submillimeter galaxies. or AGNs selected via other mid-infrared criteria. Adopting the G, M-20, and A morphological parameters, together with traditional classification boundaries, infers that three-quarters of the sample are mergers. Our sample does not, however, show any correlation between the considered morphological parameters and either infrared luminosity or AGN fractional luminosity. Moreover, the asymmetries and effective radii of our sample are distributed identically to those of massive galaxies at z similar to 2. We conclude that our sample is not preferentially associated with mergers, though a significant merger fraction is still plausible. Instead, we propose that our sample includes. examples of the massive galaxy population at z similar to 2 that harbor a briefly luminous, "flickering" AGN. and in which the G and M-20 values have been perturbed. due to either the AGN. and/or the earliest formation stages of a bulge in an inside-out manner. Furthermore, we find that the mass assembly of the central black holes in our sample leads the mass assembly of any bulge component. Finally, we speculate that our sample represents. a small fraction of the immediate antecedents of compact star-forming galaxies at z similar to 2.
WOS关键词ACTIVE GALACTIC NUCLEI ; STAR-FORMING GALAXIES ; ULTRALUMINOUS INFRARED GALAXIES ; SPITZER-SPACE-TELESCOPE ; SPECTRAL ENERGY-DISTRIBUTIONS ; INTEGRAL FIELD SPECTROSCOPY ; SUPERMASSIVE BLACK-HOLES ; EXTREMELY RED QUASARS ; UV-SELECTED GALAXIES ; SURVEY-EXPLORER WISE
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000406396300007
资助机构NASA(HST-GO-12585) ; NASA(HST-GO-12585) ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; FONDECYT(1151408) ; FONDECYT(1151408) ; NASA(HST-GO-12585) ; NASA(HST-GO-12585) ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; FONDECYT(1151408) ; FONDECYT(1151408)
源URL[http://ir.bao.ac.cn/handle/114a11/8879]  
专题国家天文台_射电天文研究部
作者单位1.Cincinnati Childrens Hosp Med Ctr, 3333 Burnet Ave, Cincinnati, OH 45229 USA
2.Univ Cape Town, Dept Astron, ZA-7700 Rondebosch, Capetown, South Africa
3.Univ Calif Los Angeles, Phys & Astron Dept, Los Angeles, CA 90095 USA
4.CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
5.Natl Radio Astron Observ, 520 Edgemont Rd, Charlottesville, VA 22903 USA
6.European Univ Cyprus, Sch Sci, Diogenes St, CY-1516 Nicosia, Cyprus
7.Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
8.Green Sci Policy Inst, Berkeley, CA 94709 USA
9.Univ Diego Portales, Fac Ingn, Nucleo Astron, Ave Ejercito Libertador 441, Santiago, Chile
10.Chalmers, Dept Space Earth & Environm, Onsala Space Observ, SE-43992 Onsala, Sweden
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GB/T 7714
Blain, Andrew,Tsai, Chao-Wei,Petty, Sara,et al. The Role of the Most Luminous Obscured AGNs in Galaxy Assembly at z similar to 2[J]. ASTROPHYSICAL JOURNAL,2017,844(2).
APA Blain, Andrew.,Tsai, Chao-Wei.,Petty, Sara.,Farrah, Duncan.,Connolly, Brian.,...&Assef, Roberto.(2017).The Role of the Most Luminous Obscured AGNs in Galaxy Assembly at z similar to 2.ASTROPHYSICAL JOURNAL,844(2).
MLA Blain, Andrew,et al."The Role of the Most Luminous Obscured AGNs in Galaxy Assembly at z similar to 2".ASTROPHYSICAL JOURNAL 844.2(2017).

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