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Scintillation Arc from FRB 20220912A
Wu, Zi-Wei1; Main, Robert A.2; Zhu, Wei-Wei1,3; Zhang, Bing4; Jiang, Peng1,5; Niu, Jia-Rui1,6; Han, Jin-Lin1,6; Li, Di1,7; Lee, Ke-Jia1,8,9; Li, Dong-Zi10; Yang, Yuan-Pei11; Wang, Fa-Yin12,13; Luo, Rui14,15; Wang, Pei1; Niu, Chen-Hui1; Xu, Heng1; Wang, Bo-Jun8,9; Wang, Wei-Yang6,8; Zhang, Yong-Kun1,6; Feng, Yi16; Zhou, De-Jiang1,6; Xu YH(徐永华)17; Deng, Can-Min18; Zhu, Yu-Hao1,6
发表期刊SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
2024-01
卷号67期号:1
DOI10.1007/s11433-023-2186-2
产权排序第17完成单位
收录类别SCI ; EI
关键词fast radio burst scintillation FRB 20220912A
摘要We present the interstellar scintillation analysis of fast radio burst (FRB) 20220912A during its extremely active episode in 2022 using data from the Five-hundred-meter Aperture Spherical Radio Telescope (FAST). We detect a scintillation arc in the FRB's secondary spectrum, which describes the power in terms of the scattered FRB signals' time delay and Doppler shift. The arc indicates that the scintillation is caused by a highly localized region. Our analysis favors a Milky Way origin of the ionized interstellar medium (IISM) for the localized scattering medium but cannot rule out a host galaxy origin. We present our method for detecting the scintillation arc, which can be applied generally to sources with irregularly spaced bursts or pulses. These methods could help shed light on the complex interstellar environment surrounding the FRBs and in our Galaxy.
资助项目National SKA Program of China[2020SKA0120200]; National SKA Program of China[2020SKA0120100]; CAS Project for Young Scientists in Basic Research[YSBR-063]; National Natural Science Foundation of China[12041303]; National Natural Science Foundation of China[11988101]; National Natural Science Foundation of China[11833009]; National Natural Science Foundation of China[11873067]; National Natural Science Foundation of China[12041304]; National Natural Science Foundation of China[12203045]; 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National SKA Program of China[2020SKA0120200, 2020SKA0120100] ; CAS Project for Young Scientists in Basic Research[YSBR-063] ; National Natural Science Foundation of China[12041303, 11988101, 11833009, 11873067, 12041304, 12203045] ; 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
文章类型Article
出版者SCIENCE PRESS
出版地16 DONGHUANGCHENGGEN NORTH ST, BEIJING 100717, PEOPLES R CHINA
ISSN1674-7348
URL查看原文
WOS记录号WOS:001127209200005
WOS研究方向Physics
WOS类目Physics, Multidisciplinary
关键词[WOS]RADIO-BURST ; PARABOLIC ARCS ; PULSAR ; SCATTERING ; EMISSION
EI入藏号20235115259598
EI主题词Scintillation
EI分类号657.2 Extraterrestrial Physics and Stellar Phenomena - 716.3 Radio Systems and Equipment - 741.1 Light/Optics
引用统计
被引频次:3[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/26509
专题射电天文研究组
作者单位1.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;
2.Max-Planck-Institut für Radioastronomie, Bonn, 53121, Germany;
3.Institute for Frontier in Astronomy and Astrophysics, Beijing Normal University, Beijing, 102206, China;
4.Nevada Center for Astrophysics and Department of Physics and Astronomy, University of Nevada, Las Vegas, NV, 89154, USA;
5.CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;
6.School of Astronomy, University of Chinese Academy of Sciences, Beijing, 100049, China;
7.NAOC-UKZN Computational Astrophysics Centre, University of KwaZulu-Natal, Durban, 4000, South Africa;
8.Department of Astronomy, Peking University, Beijing, 100871, China;
9.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing, 100871, China;
10.Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, 91125, USA;
11.South-Western Institute For Astronomy Research, Yunnan University, Kunming, 650504, China;
12.School of Astronomy and Space Science, Nanjing University, Nanjing, 210093, China;
13.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing, 210023, China;
14.CSIRO Space and Astronomy, Epping, 1710, Australia;
15.Department of Astronomy, School of Physics and Materials Science, Guangzhou University, Guangzhou, 510006, China;
16.Research Center for Intelligent Computing Platforms, Zhejiang Laboratory, Hangzhou, 311100, China;
17.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650011, China;
18.Guangxi Key Laboratory for Relativistic Astrophysics, Department of Physics, Guangxi University, Nanning, 530004, China
推荐引用方式
GB/T 7714
Wu, Zi-Wei,Main, Robert A.,Zhu, Wei-Wei,et al. Scintillation Arc from FRB 20220912A[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2024,67(1).
APA Wu, Zi-Wei.,Main, Robert A..,Zhu, Wei-Wei.,Zhang, Bing.,Jiang, Peng.,...&Zhu, Yu-Hao.(2024).Scintillation Arc from FRB 20220912A.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,67(1).
MLA Wu, Zi-Wei,et al."Scintillation Arc from FRB 20220912A".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 67.1(2024).
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