A Diverse Population of z & SIM; 2 ULIRGs Revealed by JWST Imaging
文献类型：期刊论文
| 作者 | Huang, J. -S.12,13; Li, Zi-Jian11,13; Cheng, Cheng13 ; Hou, Meicun10; Yan, Haojing9; Willner, S. P.12; Dai, Y. -S.13; Zheng, X. Z.7,8; Pan, J.6,13; Rigopoulou, D.4,5
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| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2023-06-01 |
| 卷号 | 949期号:2页码:7 |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/acc9c3 |
| 通讯作者 | Willner, S. P.(swillner@cfa.harvard.edu) |
| 英文摘要 | Four ultraluminous infrared galaxies (ULIRGs) observed with JWST/NIRcam in the Cosmos Evolution Early Release Science program offer an unbiased preview of the z & SIM; 2 ULIRG population. The objects were originally selected at 24 & mu;m and have strong polycyclic aromatic hydrocarbon emission features observed with Spitzer/Infrared Spectrometer. The four objects have similar stellar masses of & SIM;10(11) M (& ODOT;) but otherwise are quite diverse. One is an isolated disk galaxy, but it has an active nucleus as shown by X-ray observations and by a bright point-source nucleus. Two others are merging pairs with mass ratios of 6-7:1. One has active nuclei in both components, while the other has only one active nucleus: the one in the less-massive neighbor, not the ULIRG. The fourth object is clumpy and irregular and is probably a merger, but there is no sign of an active nucleus. The intrinsic spectral energy distributions for the four active galactic nuclei in these systems are typical of type-2 QSOs. This study is consistent with the idea that even if internal processes can produce large luminosities at z & SIM; 2, galaxy merging may still be necessary for the most luminous objects. The diversity of these four initial examples suggests that large samples will be needed to understand the z & SIM; 2 ULIRG population. |
| WOS关键词 | ULTRALUMINOUS INFRARED GALAXIES ; SPECTRAL ENERGY-DISTRIBUTIONS ; STAR-FORMING GALAXIES ; MAIN-SEQUENCE ; DEEP-FIELD ; EVOLUTION ; SPECTROSCOPY ; REDSHIFTS ; HERSCHEL ; STARBURST |
| 资助项目 | MOST National Key Ramp;D Program of China[2022YFA1605300] ; National Natural Science Foundation of China (NSFC)[11933003] ; National Natural Science Foundation of China (NSFC)[12273051] ; National Natural Science Foundation of China (NSFC)[11803044] ; Chinese Academy of Sciences (CAS) ; Science and Technology Facilities Council[ST/W000903/1] ; NASA/ESA/CSA James Webb Space Telescope ; NASA[NAS 5-03127] |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:001030300500001 |
| 出版者 | IOP Publishing Ltd |
| 资助机构 | MOST National Key Ramp;D Program of China ; National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Science and Technology Facilities Council ; NASA/ESA/CSA James Webb Space Telescope ; NASA |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/5310]  |
| 专题 | 研究单元未命名 |
| 通讯作者 | Willner, S. P. |
| 作者单位 | 1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 2.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210046, Peoples R China 3.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210046, Peoples R China 4.European Univ Cyprus, Sch Sci, Diogenes St, CY-1516 Nicosia, Cyprus 5.Univ Oxford, Dept Astrophys, Keble Rd, Oxford OX1 3RH, England 6.Guilin Univ Technol, Coll Earth Sci, Guilin 541004, Peoples R China 7.Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China 8.Chinese Acad Sci, Purple Mt Observ, 10 Yuanhua Rd, Nanjing 210023, Peoples R China 9.Univ Missouri, Dept Phys & Astron, Columbia, MO 65211 USA 10.Peking Univ, Kavli Inst Astron & Astrophys, Beijing, Peoples R China |
| 推荐引用方式 GB/T 7714 | Huang, J. -S.,Li, Zi-Jian,Cheng, Cheng,et al. A Diverse Population of z & SIM; 2 ULIRGs Revealed by JWST Imaging[J]. ASTROPHYSICAL JOURNAL,2023,949(2):7. |
| APA | Huang, J. -S..,Li, Zi-Jian.,Cheng, Cheng.,Hou, Meicun.,Yan, Haojing.,...&Fazio, G. G..(2023).A Diverse Population of z & SIM; 2 ULIRGs Revealed by JWST Imaging.ASTROPHYSICAL JOURNAL,949(2),7. |
| MLA | Huang, J. -S.,et al."A Diverse Population of z & SIM; 2 ULIRGs Revealed by JWST Imaging".ASTROPHYSICAL JOURNAL 949.2(2023):7. |
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