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Diverse polarization angle swings from a repeating fast radio burst source
Luo, R.1,2,3; Wang, B. J.1,2; Men, Y. P.1,2; Zhang, C. F.1,2; Jiang, J. C.1,2; Xu, H.1,2; Wang, W. Y.2,4; Lee, K. J.1,2; Han, J. L.2,4,5; Zhang, B.6; Caballero, R. N.1; Chen, M. Z.7; Chen, X. L.2,4; Gan, H. Q.2,5; Guo, Y. J.1,8; Hao, L. F.9; Huang, Y. X.9; Jiang, P.2,5; Li, H.2,4; Li, J.7; Li, Z. X.9; Luo, J. T.10; Pan, J.2; Pei, X.4,7; Qian, L.2,5; Sun, J. H.2,5; Wang, M.9; Wang, N.7; Wen, Z. G.7; Xu, R. X.1,11; Xu, Y. H.9; Yan, J.2,5; Yan, W. M.7; Yu, D. J.2,5; Yuan, J. P.7; Zhang, S. B.3,4,12; Zhu, Y.2,5
2020-10-29
Source PublicationNATURE
ISSN0028-0836
Volume586Issue:7831Pages:693-+
Contribution Rank7
AbstractFast radio bursts (FRBs) are millisecond-duration radio transients(1,2) of unknown origin. Two possible mechanisms that could generate extremely coherent emission from FRBs invoke neutron star magnetospheres(3-5) or relativistic shocks far from the central energy source(6-8). Detailed polarization observations may help us to understand the emission mechanism. However, the available FRB polarization data have been perplexing, because they show a host of polarimetric properties, including either a constant polarization angle during each burst for some repeaters(9,10) or variable polarization angles in some other apparently one-off events(11,12). Here we report observations of 15 bursts from FRB 180301 and find various polarization angle swings in seven of them. The diversity of the polarization angle features of these bursts is consistent with a magnetospheric origin of the radio emission, and disfavours the radiation models invoking relativistic shocks.
DOI10.1038/s41586-020-2827-2
Indexed BySCI
Language英语
Funding ProjectNatural Science Foundation of China[U15311243] ; Natural Science Foundation of China[11988101] ; Natural Science Foundation of China[11833009] ; Natural Science Foundation of China[11690024] ; Natural Science Foundation of China[CAS XDB23010200] ; Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS ; Max-Planck Partner Group ; Youth Innovation Promotion Association of CAS[2018075] ; NKRDPC[2017YFA0402600]
WOS Research AreaScience & Technology - Other Topics
WOS SubjectMultidisciplinary Sciences
WOS IDWOS:000623955400004
PublisherNATURE RESEARCH
Funding OrganizationNatural Science Foundation of China ; Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS ; Max-Planck Partner Group ; Youth Innovation Promotion Association of CAS ; NKRDPC
Citation statistics
Cited Times:13[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/3869
Collection射电天文研究室_天线技术实验室
射电天文研究室_数字技术实验室
Corresponding AuthorLee, K. J.; Han, J. L.; Zhang, B.
Affiliation1.Peking Univ, Kavli Inst Astron & Astrophys, Beijing, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China
3.Australia Telescope Natl Facil, CSIRO Astron & Space Sci, Epping, NSW, Australia
4.Univ Chinese Acad Sci, Sch Astron, Beijing, Peoples R China
5.Chinese Acad Sci, CAS Key Lab FAST, Natl Astron Observ, Beijing, Peoples R China
6.Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA
7.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi, Peoples R China
8.Max Planck Inst Radioastron, Bonn, Germany
9.Chinese Acad Sci, Yunnan Observ, Kunming, Yunnan, Peoples R China
10.Chinese Acad Sci, Natl Time Serv Ctr, Xian, Peoples R China
11.Peking Univ, Sch Phys, State Key Lab Nucl Phys & Technol, Beijing, Peoples R China
12.Chinese Acad Sci, Purple Mt Observ, Nanjing, Peoples R China
Recommended Citation
GB/T 7714
Luo, R.,Wang, B. J.,Men, Y. P.,et al. Diverse polarization angle swings from a repeating fast radio burst source[J]. NATURE,2020,586(7831):693-+.
APA Luo, R..,Wang, B. J..,Men, Y. P..,Zhang, C. F..,Jiang, J. C..,...&Zhu, Y..(2020).Diverse polarization angle swings from a repeating fast radio burst source.NATURE,586(7831),693-+.
MLA Luo, R.,et al."Diverse polarization angle swings from a repeating fast radio burst source".NATURE 586.7831(2020):693-+.
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