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A repeating fast radio burst associated with a persistent radio source
Niu, C-H1; Aggarwal, K.2,3; Li, D.1,4,12; Zhang, X.4,5; Chatterjee, S.6,7; Tsai, C-W1; Yu, W.5; Law, C. J.8,9; Burke-Spolaor, S.2,3,10; Cordes, J. M.6,7; Zhang, Y-K1,4; Ocker, S. K.6,7; Yao, J-M11; Wan, P.1; Feng, Y.1,4; Niino, Y.13,14; Bochenek, C.8; Cruces, M.15; Connor, L.8; Jiang, J-A16; Dai, S.17,18; Luo, R.17; Li, G-D1,4; Miao, C-C1,4; Niu, J-R1,4; Anna-Thomas, R.2,3; Sydnor, J.2,3; Stern, D.19; Wang, W-Y1,20; Yuan, M.1,4; Yue, Y-L1; Zhou, D-J1,4; Yan, Z.5; Zhu, W-W1; Zhang, B.21
2022-06-08
Source PublicationNATURE
ISSN0028-0836
Pages873-+
Contribution Rank10
AbstractThe dispersive sweep of fast radio bursts (FRBs) has been used to probe the ionized baryon content of the intergalactic medium(1), which is assumed to dominate the total extragalactic dispersion. Although the host-galaxy contributions to the dispersion measure appear to be small for most FRBs(2), in at least one case there is evidence for an extreme magneto-ionic local environment(3,4) and a compact persistent radio source(5). Here we report the detection and localization of the repeating FRB 20190520B, which is co-located with a compact, persistent radio source and associated with a dwarf host galaxy of high specific-star-formation rate at a redshift of 0.241 +/- 0.001. The estimated host-galaxy dispersion measure of approximately 903(-111)(+72 )parsecs per cubic centimetre, which is nearly an order of magnitude higher than the average of FRB host galaxies(2,6), far exceeds the dispersion-measure contribution of the intergalactic medium. Caution is thus warranted in inferring redshifts for FRBs without accurate host-galaxy identifications.
DOI10.1038/s41586-022-04755-5
Indexed BySCI
Language英语
WOS KeywordGALAXIES ; FRB
Funding ProjectNational Natural Science Foundation of China (NSFC)programme[11988101] ; National Natural Science Foundation of China (NSFC)programme[11725313] ; National Natural Science Foundation of China (NSFC)programme[12041303] ; National Natural Science Foundation of China (NSFC)programme[U1731238] ; National Natural Science Foundation of China (NSFC)programme[U2031117] ; National Natural Science Foundation of China (NSFC)programme[U1831131] ; National Natural Science Foundation of China (NSFC)programme[U1831207] ; FAST Fellowship ; National Science Foundation[2022546] ; NSF[AAG-1714897] ; NSF[YSBR-006] ; CAS Project for Young Scientists in Basic Research ; CIFAR Azrieli Global Scholar in the Gravity and the Extreme Universe programme ; JSPS KAKENHI[JP20H01942] ; Japan Society for the Promotion of Science (JSPS) KAKENHI[JP19K23456] ; Japan Society for the Promotion of Science (JSPS) KAKENHI[JP18J12714] ; Australian Research Council Discovery Early Career Award[DE210101738] ; Australian Government ; National Aeronautics and Space Administration ; W. M. Keck Foundation ; China Science and Technology Cloud (CSTCloud) ; China Environment for Network Innovations (CENI)
WOS Research AreaScience & Technology - Other Topics
WOS SubjectMultidisciplinary Sciences
WOS IDWOS:000807992000005
PublisherNATURE PORTFOLIO
Funding OrganizationNational Natural Science Foundation of China (NSFC)programme ; FAST Fellowship ; National Science Foundation ; NSF ; CAS Project for Young Scientists in Basic Research ; CIFAR Azrieli Global Scholar in the Gravity and the Extreme Universe programme ; JSPS KAKENHI ; Japan Society for the Promotion of Science (JSPS) KAKENHI ; Australian Research Council Discovery Early Career Award ; Australian Government ; National Aeronautics and Space Administration ; W. M. Keck Foundation ; China Science and Technology Cloud (CSTCloud) ; China Environment for Network Innovations (CENI)
Citation statistics
Cited Times:201[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/4806
Collection射电天文研究室_脉冲星研究团组
科研仪器设备产出_我台利用FAST观测数据文章
Corresponding AuthorLi, D.; Yu, W.; Law, C. J.
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China
2.West Virginia Univ, Dept Phys & Astron, Morgantown, WV 26506 USA
3.West Virginia Univ, Ctr Gravitat Waves & Cosmol, Morgantown, WV USA
4.Univ Chinese Acad Sci, Beijing, Peoples R China
5.Chinese Acad Sci, Shanghai Astron Observ, Shanghai, Peoples R China
6.Cornell Univ, Cornell Ctr Astrophys & Planetary Sci, Ithaca, NY USA
7.Cornell Univ, Dept Astron, Ithaca, NY 14853 USA
8.CALTECH, Cahill Ctr Astron & Astrophys, Pasadena, CA 91125 USA
9.CALTECH, Owens Valley Radio Observ, Big Pine, CA 93513 USA
10.Canadian Inst Adv Res, Toronto, ON, Canada
11.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi, Peoples R China
12.Res Ctr Intelligent Comp Platforms, Zhejiang Lab, Hangzhou, Peoples R China
13.Univ Tokyo, Grad Sch Sci, Inst Astron, Tokyo, Japan
14.Univ Tokyo, Res Ctr Earl Universe, Tokyo, Japan
15.Max Planck Inst Radioastron, Bonn, Germany
16.Univ Tokyo, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba, Japan
17.CSIRO Space & Astron, Epping, NSW, Australia
18.Western Sydney Univ, Sch Sci, Penrith, NSW, Australia
19.CALTECH, Jet Prop Lab, Pasadena, CA USA
20.Peking Univ, Sch Phys, Dept Astron, Beijing, Peoples R China
21.Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA
Recommended Citation
GB/T 7714
Niu, C-H,Aggarwal, K.,Li, D.,et al. A repeating fast radio burst associated with a persistent radio source[J]. NATURE,2022:873-+.
APA Niu, C-H.,Aggarwal, K..,Li, D..,Zhang, X..,Chatterjee, S..,...&Zhang, B..(2022).A repeating fast radio burst associated with a persistent radio source.NATURE,873-+.
MLA Niu, C-H,et al."A repeating fast radio burst associated with a persistent radio source".NATURE (2022):873-+.
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