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 |
DOI | 10.1007/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 |
ISSN | 1674-7348 |
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 | |
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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