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Giant Micropulse Emission in the Vela Pulsar at the C Band
Chen, J. L.1; Wen, Z. G.2,3; Hao, L. F.4; Yuan, J. P.2,3; Li, J.2,3,5; Wang, H. G.2,6; Yan, W. M.2,3; Lee, K. J.7; Wang, N.2,3; Xu, Y. H.4; Li, Z. X.4; Huang, Y. X.4; Yuen, R.2; Mijit, M.8
2020-08-01
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume899Issue:2Pages:118
Contribution Rank2
AbstractWe present here the analysis of giant micropulses from the Vela pulsar. A total of 4187 giant micropulses with peak flux density >2.5 Jy were detected during almost 4 hr of observations carried out with the Yunnan 40 m radio telescope at 6800 MHz. Nine of the giant micropulses arrived approximately 3-4 ms earlier than the peak of average pulse profile, longer than that at lower frequencies. The remaining giant micropulses were clustered into three distributions that correspond to three main emission regions, including four giant micropulses occurring on the trailing edge of the averaged profile. We find that the peak flux density distribution follows a power law with index alpha -4. Furthermore, a certain amount of memory is present from the giant micropulse waiting time distribution. Possible emission mechanisms are discussed.
KeywordRadio pulsars
DOI10.3847/1538-4357/aba2e8
URL查看原文
Indexed BySCI
Language英语
WOS KeywordRADIO PULSES ; SINGLE-PULSE ; SPECTRA
Funding ProjectWest Light Foundation of Chinese Academy of Sciences[WLFC 2016-QNXZ-B-24] ; Chinese National Science Foundation[U1838109] ; Chinese National Science Foundation[U1731238] ; Chinese National Science Foundation[U1831102] ; Chinese National Science Foundation[U1631106] ; Chinese National Science Foundation[11873080] ; National Basic Research Program of China (973 Program)[2015CB857100] ; prospective project of the Astronomical Research Center of the Chinese Academy of Sciences ; National Program on Key Research and Development Project[2016YFA0400804] ; 2018 project of Xinjiang uygur autonomous region of China ; Scientific and Technological Innovation Programs of Higher Education Institutions in Shanxi[2019L0863]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000563106400001
PublisherIOP PUBLISHING LTD
Funding OrganizationWest Light Foundation of Chinese Academy of Sciences ; Chinese National Science Foundation ; National Basic Research Program of China (973 Program) ; prospective project of the Astronomical Research Center of the Chinese Academy of Sciences ; National Program on Key Research and Development Project ; 2018 project of Xinjiang uygur autonomous region of China ; Scientific and Technological Innovation Programs of Higher Education Institutions in Shanxi
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Cited Times:6[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/3624
Collection射电天文研究室_脉冲星研究团组
110米口径全可动射电望远镜(QTT)_110米大口径全可动射电望远镜关键技术研究(973项目)_课题4:反射面高精度快速测量与主动面实时闭环修正
Corresponding AuthorWen, Z. G.
Affiliation1.Yuncheng Univ, Dept Phys & Elect Engn, Yuncheng 044000, Shanxi, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, 150,Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
3.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China
4.Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Yunnan, Peoples R China
5.Key Lab Microwave Technoloty, Urumqi 830011, Xinjiang, Peoples R China
6.Guangzhou Univ, Sch Phys & Elect Engn, Guangzhou 510006, Peoples R China
7.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
8.Xinjiang Univ, Sch Phys, Urumqi 830046, Peoples R China
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Chen, J. L.,Wen, Z. G.,Hao, L. F.,et al. Giant Micropulse Emission in the Vela Pulsar at the C Band[J]. ASTROPHYSICAL JOURNAL,2020,899(2):118.
APA Chen, J. L..,Wen, Z. G..,Hao, L. F..,Yuan, J. P..,Li, J..,...&Mijit, M..(2020).Giant Micropulse Emission in the Vela Pulsar at the C Band.ASTROPHYSICAL JOURNAL,899(2),118.
MLA Chen, J. L.,et al."Giant Micropulse Emission in the Vela Pulsar at the C Band".ASTROPHYSICAL JOURNAL 899.2(2020):118.
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