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Very Long Baseline Array Observations of Parsec-scale Radio Emission in Dual Active Galactic Nuclei
Xu, Wancheng1,2; Cui, Lang1,3,4; Liu, Xiang1,3,4; An, Tao5; Cao, Hongmin6; Jiang, Pengfei1; Ho, Luis C.7,8; Chang, Ning1; Yang, Xiaolong5; Shen, Yuling1; Tan, Guiping1; Han, Zhenhua9; Fan, Junhui10; Zhang, Ming1,3,4
2024-07-01
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume969Issue:1Pages:36
Contribution Rank1
AbstractIt is believed that dual active galactic nuclei (AGN) form during galaxy mergers. Studying dual-AGN emission can provide valuable insights into galaxy merging and evolution. To investigate parsec-scale radio emission properties, we observed eight radio components of four selected dual-AGN systems using the Very Long Baseline Array (VLBA) at 5 GHz in multiple-phase-center mode. Among them, two compact radio components, labeled J0051+0020B and J2300-0005A, were detected clearly on parsec scales for the first time. However, the radio emission of the other six components was resolved out in the high-resolution images. We provide the values or upper limits of the brightness temperature and radio emission power, and analyze the emission origins in detail for each target. Based on their physical properties reported in this work and in the literature, we suggest that the radio emission in J0051+0020B and J2300-0005A originates primarily from compact jets, while the other six sources show more complex emission mechanisms. In addition, our VLBA observations suggest that the systematic X-ray deficit in our dual-AGN sample is likely attributed to the tidally induced effect and possibly a viewing angle effect.
DOI10.3847/1538-4357/ad463b
Indexed BySCI
Language英语
WOS KeywordDIGITAL SKY SURVEY ; BINARY BLACK-HOLE ; ENHANCED STAR-FORMATION ; PALOMAR-GREEN QUASARS ; SURVEY STRIPE 82 ; SDSS-IV MANGA ; X-RAY ; VLBI OBSERVATIONS ; OFF-NUCLEUS ; GALAXY PAIRS
Funding ProjectCAS Light of West China Program[2021-XBQNXZ-005] ; National SKA Program of China[2022SKA0120102] ; National Key RD Program[2018YFA0404602] ; National Key RD Program[2023YFE0102300] ; Tianshan Talent Training Program[2023TSYCCX0099] ; Xinjiang Tianchi Talent Program ; Urumqi Nanshan Astronomy and Deep Space Exploration Observation and Research Station of Xinjiang[XJYWZ2303] ; National Science Foundation of China[11721303] ; National Science Foundation of China[11991052] ; National Science Foundation of China[12011540375] ; National Science Foundation of China[12233001] ; National Key R&D Program of China[2022YFF0503401] ; China Manned Space Project[CMS-CSST-2021-A04] ; China Manned Space Project[CMS-CSST-2021-A06] ; China Manned Space Project[BL255A] ; China Manned Space Project[BL255B]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001256803900001
PublisherIOP Publishing Ltd
Funding OrganizationCAS Light of West China Program ; National SKA Program of China ; National Key RD Program ; Tianshan Talent Training Program ; Xinjiang Tianchi Talent Program ; Urumqi Nanshan Astronomy and Deep Space Exploration Observation and Research Station of Xinjiang ; National Science Foundation of China ; National Key R&D Program of China ; China Manned Space Project
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Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/6793
Collection射电天文研究室_星系宇宙学研究团组
Corresponding AuthorCui, Lang
Affiliation1.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China
2.Univ Chinese Acad Sci, Coll Astron & Space Sci, 1 Yanqihu East Rd, Beijing 101408, Peoples R China
3.Chinese Acad Sci, Key Lab Radio Astron, 150 Sci 1 St, Urumqi 830011, Peoples R China
4.Xinjiang Key Lab Radio Astrophys, 150 Sci 1 St, Urumqi 830011, Peoples R China
5.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
6.Shangqiu Normal Univ, Sch Elect & Elect Engn, 298 Wenhua Rd, Shangqiu 476000, Henan, Peoples R China
7.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
8.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China
9.Xinjiang Normal Univ, Coll Phys & Elect Engn, 102 Xinyi Rd, Urumqi 830054, Peoples R China
10.Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Xu, Wancheng,Cui, Lang,Liu, Xiang,et al. Very Long Baseline Array Observations of Parsec-scale Radio Emission in Dual Active Galactic Nuclei[J]. ASTROPHYSICAL JOURNAL,2024,969(1):36.
APA Xu, Wancheng.,Cui, Lang.,Liu, Xiang.,An, Tao.,Cao, Hongmin.,...&Zhang, Ming.(2024).Very Long Baseline Array Observations of Parsec-scale Radio Emission in Dual Active Galactic Nuclei.ASTROPHYSICAL JOURNAL,969(1),36.
MLA Xu, Wancheng,et al."Very Long Baseline Array Observations of Parsec-scale Radio Emission in Dual Active Galactic Nuclei".ASTROPHYSICAL JOURNAL 969.1(2024):36.
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