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Scintillation Velocity and Arc Observations of FRB 20201124A
Wu, Ziwei1; Zhu, Weiwei1,2; Zhang, Bing3,4; Feng, Yi5; Han, JinLin1,6; Li, Di1,7,8; Li, Dongzi9; Luo, Rui10; Niu, Chenhui11; Niu, Jiarui1,6; Wang, Bojun1; Wang, Fayin12,13; Wang, Pei1; Wang, Weiyang14; Xu, Heng1; Yang, Yuanpei15; Zhang, Yongkun1,6; Zhou, Dejiang1,6; Zhu, Yuhao1,6; Deng, Can-Min16; Xu YH(徐永华)17
发表期刊ASTROPHYSICAL JOURNAL LETTERS
2024-07-01
卷号969期号:1
DOI10.3847/2041-8213/ad5979
产权排序第17完成单位
收录类别SCI
摘要We present the scintillation velocity measurements of FRB 20201124A from the Five-hundred-meter Aperture Spherical radio Telescope observations, which reveal an annual variation. This annual variation is further supported by changes detected in the scintillation arc as observed from the secondary spectrum. We attribute the annual velocity variation to the presence of a moderately anisotropic scattering screen located at a distance of 0.4 +/- 0.1 kpc from Earth. Our results prove that the scintillation of this fast radio burst (FRB) is mainly caused by material close to Earth on a Galactic scale. However, scintillation observations of other FRBs may expose their surrounding environment or uncover possible orbital motion if scintillation is caused by materials in their host galaxy.
资助项目China Postdoctoral Science Foundation[2023M743517]; National SKA Program of China[2020SKA0120200]; National SKA Program of China[2020SKA0120100]; CAS Project for Young Scientists in Basic Research[YSBR-063]; National Nature Science Foundation[12041303]; National Nature Science Foundation[11988101]; National Nature Science Foundation[11833009]; National Nature Science Foundation[11873067]; National Nature Science Foundation[12041304]; National Nature Science Foundation[12273009]; National Nature Science Foundation[12203045]; National Nature Science Foundation[12203013]; National Nature Science Foundation[12303042]; National Key R&D Program of China[2017YFA0402600]; National Key R&D Program of China[2021YFA0718500]; National Key R&D Program of China[2017YFA0402602]; National Key R&D Program of China[2022YFC2205203]; CAS-MPG LEGACY project; Max-Planck Partner Group; Key Research Project of Zhejiang Lab[2021PE0AC0]; Western Light Youth Project of Chinese Academy of Sciences
项目资助者China Postdoctoral Science Foundation[2023M743517] ; National SKA Program of China[2020SKA0120200, 2020SKA0120100] ; CAS Project for Young Scientists in Basic Research[YSBR-063] ; National Nature Science Foundation[12041303, 11988101, 11833009, 11873067, 12041304, 12273009, 12203045, 12203013, 12303042] ; National Key R&D Program of China[2017YFA0402600, 2021YFA0718500, 2017YFA0402602, 2022YFC2205203] ; CAS-MPG LEGACY project ; Max-Planck Partner Group ; Key Research Project of Zhejiang Lab[2021PE0AC0] ; Western Light Youth Project of Chinese Academy of Sciences
语种英语
学科领域天文学 ; 射电天文学
文章类型Article
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN2041-8205
URL查看原文
WOS记录号WOS:001260096700001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]LARGE EUROPEAN ARRAY ; INTERSTELLAR SCINTILLATION ; RADIO-BURST ; INTRADAY VARIABILITY ; MULTIPLE-SCATTERING ; ANNUAL MODULATION ; PARABOLIC ARCS ; PULSARS ; SCINTILLOMETRY ; PSRCHIVE
引用统计
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/27437
专题射电天文研究组
作者单位1.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China; [email protected], [email protected];
2.Institute for Frontier in Astronomy and Astrophysics, Beijing Normal University, Beijing 102206, People's Republic of China;
3.Nevada Center for Astrophysics, University of Nevada, Las Vegas, NV 89154, USA;
4.Department of Physics and Astronomy, University of Nevada, Las Vegas, NV 89154, USA;
5.Research Center for Astronomical Computing, Zhejiang Laboratory, Hangzhou 311100, People's Republic of China;
6.School of Astronomy, University of Chinese Academy of Sciences, Beijing, People's Republic of China;
7.NAOC-UKZN Computational Astrophysics Centre, University of KwaZulu-Natal, Durban 4000, South Africa;
8.Research Center for Intelligent Computing Platforms, Zhejiang Laboratory, Hangzhou 311100, People's Republic of China;
9.Cahill Center for Astronomy and Astrophysics, MC 249-17 California Institute of Technology, Pasadena, CA 91125, USA;
10.Department of Astronomy, School of Physics and Materials Science, Guangzhou University, Guangzhou 510006, People's Republic of China;
11.Institute of Astrophysics, Central China Normal University, Wuhan 430079, People's Republic of China;
12.School of Astronomy and Space Science, Nanjing University, Nanjing 210093, People's Republic of China;
13.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210093​, People's Republic of China;
14.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China;
15.South-Western Institute For Astronomy Research, Yunnan University, Yunnan 650504, People's Republic of China;
16.Guangxi Key Laboratory for Relativistic Astrophysics, Department of Physics, Guangxi University, Nanning 530004, People's Republic of China;
17.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, People's Republic of China
推荐引用方式
GB/T 7714
Wu, Ziwei,Zhu, Weiwei,Zhang, Bing,et al. Scintillation Velocity and Arc Observations of FRB 20201124A[J]. ASTROPHYSICAL JOURNAL LETTERS,2024,969(1).
APA Wu, Ziwei.,Zhu, Weiwei.,Zhang, Bing.,Feng, Yi.,Han, JinLin.,...&徐永华.(2024).Scintillation Velocity and Arc Observations of FRB 20201124A.ASTROPHYSICAL JOURNAL LETTERS,969(1).
MLA Wu, Ziwei,et al."Scintillation Velocity and Arc Observations of FRB 20201124A".ASTROPHYSICAL JOURNAL LETTERS 969.1(2024).
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