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Frequency-dependent polarization of repeating fast radio bursts implications for their origin
Feng, Yi1,2,3; Li, Di1,2,4; Yang, Yuan-Pei5; Zhang, Yongkun1,3; Zhu, Weiwei1; Zhang, Bing6,7; Lu, Wenbin8; Wang, Pei1; Dai, Shi9; Lynch, Ryan S.10; Yao, Jumei11; Jiang, Jinchen1,12; Niu, Jiarui1,3; Zhou, Dejiang1,3; Xu, Heng1,12; Miao, Chenchen1,3; Niu, Chenhui1; Meng, Lingqi1,3; Qian, Lei1; Tsai, Chao-Wei1; Wang, Bojun1,12; Xue, Mengyao1; Yue, Youling1; Yuan, Mao1,3; Zhang, Songbo13; Zhang, Lei1
2022-03-18
Source PublicationSCIENCE
ISSN0036-8075
Volume375Issue:6586Pages:1266-+
Contribution Rank11
AbstractThe polarization of fast radio bursts (FRBs), which are bright astronomical transient phenomena, contains information about their environments. Using wide-band observations with two telescopes, we report polarization measurements of five repeating FRBs and find a trend of lower polarization at lower frequencies. This behavior is modeled as multipath scattering, characterized by a single parameter, sigma(Rm), the rotation measure (RM) scatter. Sources with higher sigma(Rm) have higher RM magnitude and scattering time scales. The two sources with the highest sigma(Rm), FRB 20121102A and FRB 20190520B, are associated with compact persistent radio sources. These properties indicate a complex environment near the repeating FRBs, such as a supernova remnant or a pulsar wind nebula, consistent with their having arisen from young stellar populations.
DOI10.1126/science.abl7759
Indexed BySCI
Language英语
WOS KeywordCIRCULAR-POLARIZATION ; PULSARS ; POLARIMETRY
Funding ProjectNSFC[11988101] ; NSFC[11725313] ; NSFC[12003028] ; NSFC[12041303] ; NSFC[11873067] ; NSFC[U2031117] ; NSFC[12041306] ; NSFC[11903049] ; NSFC[12103069] ; National Key R&D Program of China[2017YFA0402600] ; Key Research Project of Zhejiang Lab[2021PE0AC03] ; National SKA Program of China[2020SKA0120200] ; Lyman Spitzer, Jr. Fellowship at Princeton University ; Youth Innovation Promotion Association CAS[2021055] ; CAS Project for Young Scientists in Basic Research[YSBR-006] ; Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS ; Australian Research Council Discovery Early Career Award - Australian Government[DE210101738] ; Youth Innovation Promotion Association of CAS[2018075] ; China Postdoctoral Science Foundation[2020M681758]
WOS Research AreaScience & Technology - Other Topics
WOS SubjectMultidisciplinary Sciences
WOS IDWOS:000770386600035
PublisherAMER ASSOC ADVANCEMENT SCIENCE
Funding OrganizationNSFC ; National Key R&D Program of China ; Key Research Project of Zhejiang Lab ; National SKA Program of China ; Lyman Spitzer, Jr. Fellowship at Princeton University ; Youth Innovation Promotion Association CAS ; CAS Project for Young Scientists in Basic Research ; Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS ; Australian Research Council Discovery Early Career Award - Australian Government ; Youth Innovation Promotion Association of CAS ; China Postdoctoral Science Foundation
Citation statistics
Cited Times:102[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/4588
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, Di
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
2.Zhejiang Lab, Hangzhou 311121, Zhejiang, Peoples R China
3.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China
4.Univ KwaZulu Natal, Chinese Acad Sci, Natl Astron Observ, Computat Astrophys Ctr, ZA-4000 Durban, South Africa
5.Yunnan Univ, South Western Inst Astron Res, Kunming 650504, Yunnan, Peoples R China
6.Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA
7.Univ Nevada, Nevada Ctr Astrophys, Las Vegas, NV 89154 USA
8.Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
9.Western Sydney Univ, Sch Sci, Penrith, NSW 2751, Australia
10.Green Bank Observ, Green Bank, WV 24401 USA
11.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
12.Peking Univ, Sch Phys, Beijing 100871, Peoples R China
13.Chinese Acad Sci, Purple Mt Observ, Nanjing 210023, Peoples R China
Recommended Citation
GB/T 7714
Feng, Yi,Li, Di,Yang, Yuan-Pei,et al. Frequency-dependent polarization of repeating fast radio bursts implications for their origin[J]. SCIENCE,2022,375(6586):1266-+.
APA Feng, Yi.,Li, Di.,Yang, Yuan-Pei.,Zhang, Yongkun.,Zhu, Weiwei.,...&Zhang, Lei.(2022).Frequency-dependent polarization of repeating fast radio bursts implications for their origin.SCIENCE,375(6586),1266-+.
MLA Feng, Yi,et al."Frequency-dependent polarization of repeating fast radio bursts implications for their origin".SCIENCE 375.6586(2022):1266-+.
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