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Observational Evidence for a Correlation between the Magnetic Field of Jets and Star Formation Rate in Host Galaxies
Chen, Yongyun1; Gu, Qiusheng2; Fan, Junhui3; Guo, Xiaotong4; Yu, Xiaoling1; Ding, Nan5; Xiong DR(熊定荣)6
发表期刊ASTROPHYSICAL JOURNAL
2025-01-10
卷号978期号:2
DOI10.3847/1538-4357/ad9b8a
产权排序第6完成单位
收录类别SCI
摘要Accretion supermassive black holes in the center of active galaxies usually produce jet-collimated bipolar outflows of relativistic particles. Magnetic fields near the black hole event horizon may play a crucial role in the formation of jets/outflows. Both theory and observation indicate that jets/outflows driven by centrally active supermassive black holes have a feedback effect on the overall properties of the host galaxies. Therefore, the magnetic field is a key ingredient for the formation and evolution of galaxies. Here, we report a clear correlation between the magnetic field of jets and star formation rate for a large sample of 96 galaxies hosting supermassive black holes, which suggests that the star formation of active galactic nuclei host galaxies may be powered by the jets.
资助项目National Natural Science Foundation of China (NSFC)[11733001]; National Natural Science Foundation of China (NSFC)[U2031201]; National Natural Science Foundation of China (NSFC)[12433004]; National Natural Science Foundation of China[2081450001]; Yunnan Province[CMS-CSST-2021-A05]; China Manned Space Project[12303017]; National Nature Science Foundation of China[2308085QA33]; Anhui Provincial Natural Science Foundation[12473020]; NSFC[YNWR-QNBJ-2020-116]; Yunnan Province Youth Top Talent Project
项目资助者National Natural Science Foundation of China (NSFC)[11733001, U2031201, 12433004] ; National Natural Science Foundation of China[2081450001] ; Yunnan Province[CMS-CSST-2021-A05] ; China Manned Space Project[12303017] ; National Nature Science Foundation of China[2308085QA33] ; Anhui Provincial Natural Science Foundation[12473020] ; NSFC[YNWR-QNBJ-2020-116] ; Yunnan Province Youth Top Talent Project
语种英语
学科领域天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学
文章类型Article
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS记录号WOS:001389215900001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]ACTIVE GALACTIC NUCLEI ; SMALL-SCALE DYNAMO ; ENERGY ; FEEDBACK ; STELLAR ; DUST ; EMISSION ; OPACITY ; MODEL ; IV
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文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/27961
专题南方基地
作者单位1.College of Physics and Electronic Engineering, Qujing Normal University, Qujing 655011, People's Republic of China;
2.School of Astronomy and Space Science, Nanjing University, Nanjing 210093, People's Republic of China;
3.Center for Astrophysics, Guangzhou University, Guangzhou 510006, People's Republic of China;
4.Anqing Normal University, Anhui 246133, People's Republic of China;
5.School of Physical Science and Technology, Kunming University, Kunming 650214, People's Republic of China;
6.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, People's Republic of China
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Chen, Yongyun,Gu, Qiusheng,Fan, Junhui,et al. Observational Evidence for a Correlation between the Magnetic Field of Jets and Star Formation Rate in Host Galaxies[J]. ASTROPHYSICAL JOURNAL,2025,978(2).
APA Chen, Yongyun.,Gu, Qiusheng.,Fan, Junhui.,Guo, Xiaotong.,Yu, Xiaoling.,...&熊定荣.(2025).Observational Evidence for a Correlation between the Magnetic Field of Jets and Star Formation Rate in Host Galaxies.ASTROPHYSICAL JOURNAL,978(2).
MLA Chen, Yongyun,et al."Observational Evidence for a Correlation between the Magnetic Field of Jets and Star Formation Rate in Host Galaxies".ASTROPHYSICAL JOURNAL 978.2(2025).
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