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The relation between black hole spin and star formation in massive star-forming galaxies

文献类型：期刊论文

作者Chen, Yongyun4; Gu, Qiusheng3; Fan, Junhui5; Xiong DR(熊定荣)2; Yu, Xiaoling4; Ding, Nan1; Guo, Xiaotong6
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2025-02-22
卷号537期号:4页码:3595-3602
关键词galaxies:active galaxies: formation galaxies: general galaxies:jets
ISSN号0035-8711
DOI10.1093/mnras/staf275
产权排序第4完成单位
文献子类Article
英文摘要It has always been believed that feedback from active galactic nuclei (AGNs) has an important impact on star formation in massive galaxies. Black hole spin is an important physical parameter of AGN. We use a large sample of massive star-forming galaxies to study the effects of AGN on star formation. Our main results are as follows: (i) there are significant correlations between black hole spin and star formation rate, specific star formation rate, and star formation activity parameter for massive star-forming early- and late-type galaxies, respectively. These results indicate that the spin of supermassive black holes regulates the star formation of massive star-forming early- and late-type galaxies. (2) The slopes of the relationship between black hole spin and star formation rate, specific star formation rate, and star formation activity parameter for massive star-forming early- and late-type galaxies are similar within the error range. These results imply that the mechanism of black hole spin regulating star formation may be similar in massive star-forming early-type and late-type galaxies.
学科主题天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学
URL标识查看原文
出版地GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
WOS关键词ACTIVE GALACTIC NUCLEI ; EDDINGTON ACCRETION DISKS ; DIGITAL SKY SURVEY ; JET POWER ; OBSERVATIONAL EVIDENCE ; FORMATION RATES ; MOLECULAR GAS ; AGN FEEDBACK ; RADIO JETS ; EVOLUTION
资助项目National Natural Science Foundation of China[11733001]; National Natural Science Foundation of China[U2031201]; National Natural Science Foundation of China[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; CAS Light of West China Program
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001428162300001
出版者OXFORD UNIV PRESS
资助机构National Natural Science Foundation of China[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 ; CAS Light of West China Program
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28185]  
专题云南天文台_丽江天文观测站（南方基地）
作者单位1.School of Physical Science and Technology, Kunming University, Kunming 650214, P. R. China;
2.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China;
3.School of Astronomy and Space Science, Nanjing University, Nanjing 210093, P. R. China;
4.College of Physics and Electronic Engineering, Qujing Normal University, Qujing 655011, P. R. China;
5.Center for Astrophysics,Guang zhou University, Guang zhou 510006, China;
6.School of Mathematics and Physics, Anqing Normal University, Anqing 246011, P. R. China
推荐引用方式
GB/T 7714		 Chen, Yongyun,Gu, Qiusheng,Fan, Junhui,et al. The relation between black hole spin and star formation in massive star-forming galaxies[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2025,537(4):3595-3602.
APA Chen, Yongyun.,Gu, Qiusheng.,Fan, Junhui.,熊定荣.,Yu, Xiaoling.,...&Guo, Xiaotong.(2025).The relation between black hole spin and star formation in massive star-forming galaxies.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,537(4),3595-3602.
MLA Chen, Yongyun,et al."The relation between black hole spin and star formation in massive star-forming galaxies".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 537.4(2025):3595-3602.

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