Institutional Repository of Radio Astronomy Research Laboratory
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![]() ![]() | |
2022-06-08 | |
Source Publication | NATURE
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ISSN | 0028-0836 |
Pages | 873-+ |
Contribution Rank | 10 |
Abstract | The 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. |
DOI | 10.1038/s41586-022-04755-5 |
Indexed By | SCI |
Language | 英语 |
WOS Keyword | GALAXIES ; FRB |
Funding Project | National 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 Area | Science & Technology - Other Topics |
WOS Subject | Multidisciplinary Sciences |
WOS ID | WOS:000807992000005 |
Publisher | NATURE PORTFOLIO |
Funding Organization | National 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 | |
Document Type | 期刊论文 |
Identifier | http://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 Author | Li, D.; Yu, W.; Law, C. J. |
Affiliation | 1.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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