中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Unveiling the Small-scale Jets in the Rapidly Growing Supermassive Black Hole IZw1

文献类型:期刊论文

作者Yang, Xiaolong10,11,12; Yao, Su9; Gallo, Luigi C.8; Yang, Jun7; Ho, Luis C.6,11; Gu, Minfeng5; Baan, Willem A.3,4; Svoboda, Jiri2; Wang, Ran6,11; Liu, Xiang4
刊名ASTROPHYSICAL JOURNAL
出版日期2024-05-01
卷号966期号:2页码:151
ISSN号0004-637X
DOI10.3847/1538-4357/ad343c
产权排序10
英文摘要Accretion of black holes at near-Eddington or super-Eddington rates represents the most powerful episode driving black hole growth, potentially occurring across various types of objects. However, the physics governing accretion and jet-disk coupling in such states remains unclear, primarily due to the difficulty in detecting associated jets, which may emit extremely weakly or exhibit episodic behavior. Only a few near/super-Eddington systems have demonstrated radio activity, and it remains uncertain whether jets exist and what their properties are in super-Eddington active galactic nuclei (AGNs) and ultraluminous X-ray sources. This uncertainty stems mainly from the complex radio emission mix, which includes contributions from jets, star formation activity, photoionized gas, accretion disk wind, and coronal activity. In this work, we conducted high-resolution, very long baseline interferometry observations to investigate jets in the highly accreting narrow-line Seyfert I system I Zw 1. Our observations successfully revealed small-scale jets (with a linear size of similar to 45 pc) at both 1.5 and 5 GHz, based on the high radio brightness temperature, radio morphology, and spectral index distribution. Additionally, the parsec-scale jet observed in I Zw 1 displays a knotted morphology reminiscent of other sources accreting at similar rates. In summary, the high accretion rates and jet properties observed in the AGN I Zw 1 may support the AGN/X-ray binary analogy in this extreme state.
WOS关键词LINE SEYFERT 1 ; ACTIVE GALACTIC NUCLEI ; ADVECTION-DOMINATED ACCRETION ; COMPACT STEEP-SPECTRUM ; LONGER XMM-NEWTON ; X-RAY BINARIES ; I ZWICKY 1 ; STAR-FORMATION ; UNIFIED MODEL ; MOLECULAR GAS
资助项目National Science Foundation of China ; National Key R&D Program of China[2016YFA0400702] ; National Key R&D Program of China[2018YFA0404602] ; National Key R&D Program of China[2018YFA0404603] ; Shanghai Sailing Program[21YF1455300] ; China Postdoctoral Science Foundation[2021M693267] ; Alexander von Humboldt Foundation Fellowship ; Czech Science Foundation ; Shanghai Pilot Program for Basic Research Chinese Academy of Science, Shanghai Branch[JCYJ-SHFY-2021-013] ; National SKA Program of China[2022SKA0120102] ; China Manned Space Project[CMSCSST-2021-A06] ; China Manned Space Project[EY037] ; China Manned Space Project[BY145] ; North American radio astronomy institutes[23 23] ; [12103076] ; [11721303] ; [11991052]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001221176500001
出版者IOP Publishing Ltd
资助机构National Science Foundation of China ; National Key R&D Program of China ; Shanghai Sailing Program ; China Postdoctoral Science Foundation ; Alexander von Humboldt Foundation Fellowship ; Czech Science Foundation ; Shanghai Pilot Program for Basic Research Chinese Academy of Science, Shanghai Branch ; National SKA Program of China ; China Manned Space Project ; North American radio astronomy institutes
源URL[http://ir.xao.ac.cn/handle/45760611-7/6616]  
专题恒星形成与演化研究团组
星系宇宙学研究团组
通讯作者Yang, Xiaolong
作者单位1.Univ Chinese Acad Sci, 19A Yuquanlu, Beijing 100049, Peoples R China
2.Acad Sci, Astron Inst, Bocni II 1401, Prague 14131, Czech Republic
3.Netherlands Inst Radio Astron ASTRON, NL-7991 PD Dwingeloo, Netherlands
4.Chinese Acad Sci, Key Lab Radio Astron, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China
5.Chinese Acad Sci, Key Lab Res Galaxies & Cosmol, Shanghai Astron Observ, Shanghai 200030, Peoples R China
6.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China
7.Chalmers Univ Technol, Dept Space Earth & Environm, Onsala Space Observ, SE-43992 Onsala, Sweden
8.St Marys Univ, Dept Astron & Phys, Halifax, NS B3H 3C3, Canada
9.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
10.Shanghai Key Lab Space Nav & Positioning Tech, Shanghai 200030, Peoples R China
推荐引用方式
GB/T 7714
Yang, Xiaolong,Yao, Su,Gallo, Luigi C.,et al. Unveiling the Small-scale Jets in the Rapidly Growing Supermassive Black Hole IZw1[J]. ASTROPHYSICAL JOURNAL,2024,966(2):151.
APA Yang, Xiaolong.,Yao, Su.,Gallo, Luigi C..,Yang, Jun.,Ho, Luis C..,...&Zhao, Wei.(2024).Unveiling the Small-scale Jets in the Rapidly Growing Supermassive Black Hole IZw1.ASTROPHYSICAL JOURNAL,966(2),151.
MLA Yang, Xiaolong,et al."Unveiling the Small-scale Jets in the Rapidly Growing Supermassive Black Hole IZw1".ASTROPHYSICAL JOURNAL 966.2(2024):151.

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