中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Individual pulse emission from the diffuse drifter PSR J1401-6357 using the ultrawideband receiver on the Parkes radio telescope

文献类型:期刊论文

作者Chen, J. L.7; Wen, Z. G.3,4,5,6; Duan, X. F.4,6; He, D. L.6; Wang, N.5,6; Wang, H. G.2,6; Yuen, R.6; Yuan, J. P.5,6; Yan, W. M.5,6; Wang, Z.1,6
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2023-02-01
卷号519期号:2页码:2709-2717
ISSN号0035-8711
关键词stars: neutron pulsars: general pulsars: individual (J1401-6357)
DOI10.1093/mnras/stac3654
通讯作者Wen, Z. G.(wenzhigang@xao.ac.cn)
英文摘要In this study, we report on a detailed single pulse analysis of the radio emission from the pulsar J1401 - 6357 (B1358 - 63) based on data observed with the ultrawideband low-frequency receiver on the Parkes radio telescope. In addition to a weak leading component, the integrated pulse profile features a single-humped structure with a slight asymmetry. The frequency evolution of the pulse profile is studied. Well-defined nulls, with an estimated nulling fraction greater than 2 per cent, are present across the whole frequency band. No emission is detected with significance above 3 sigma in the average pulse profile integrated over all null pulses. Using fluctuation spectral analysis, we reveal the existence of temporal-dependent subpulse drifting in this pulsar for the first time. A clear double-peaked feature is present at exactly the alias border across the whole frequency band, which suggests that the apparent drift sense changes during the observation. Our observations provide further confirmation that the phenomena of pulse nulling and subpulse drifting are independent of observing frequency, which suggest that they invoke changes on the global magnetospheric scale.
WOS关键词SUBPULSE MODULATION ; FREQUENCY-DEPENDENCE ; FLUCTUATION SPECTRA ; EMPIRICAL-THEORY ; MAGNETIC-FIELD ; BEHAVIOR ; MECHANISM ; EVOLUTION ; NULLS ; MODEL
资助项目National Key Research and Development Program of China[2022YFC2205203] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-1] ; National Natural Science Foundation of China[11988101] ; National Natural Science Foundation of China[U1838109] ; National Natural Science Foundation of China[12041304] ; National Natural Science Foundation of China[12041301] ; National Natural Science Foundation of China[11873080] ; National Natural Science Foundation of China[12133004] ; National Natural Science Foundation of China[U1631106] ; National SKA Program of China[2020SKA0120100] ; Chinese Academy of Sciences Foundation of the young scholars of western[2020-XBQNXZ-019] ; Xinjiang Key Laboratory of Radio Astrophysics[2022D04058] ; Natural Science Foundation of Shanxi Province[20210302123083] ; Scientific and Technological Innovation Programs of Higher Education Institutions in Shanxi[2021L480] ; CAS[2018] ; project of Xinjiang uygur autonomous region of China ; student innovation project of Yuncheng university[20220940] ; Australian Government
WOS研究方向Astronomy & Astrophysics
语种英语
出版者OXFORD UNIV PRESS
WOS记录号WOS:000910908900030
资助机构National Key Research and Development Program of China ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; National Natural Science Foundation of China ; National SKA Program of China ; Chinese Academy of Sciences Foundation of the young scholars of western ; Xinjiang Key Laboratory of Radio Astrophysics ; Natural Science Foundation of Shanxi Province ; Scientific and Technological Innovation Programs of Higher Education Institutions in Shanxi ; CAS ; project of Xinjiang uygur autonomous region of China ; student innovation project of Yuncheng university ; Australian Government
源URL[http://ir.xao.ac.cn/handle/45760611-7/5055]  
专题脉冲星研究团组
通讯作者Wen, Z. G.
作者单位1.Xinjiang Univ, Sch Phys Sci & Technol, Urumqi 830046, Xinjiang, Peoples R China
2.Guangzhou Univ, Sch Phys & Elect Engn, Guangzhou 510006, Peoples R China
3.Guizhou Prov Key Lab Radio Astron & Data Proc, Guiyang 550001, Guizhou, Peoples R China
4.Key Lab Microwave Technol, Urumqi 830011, Xinjiang, Peoples R China
5.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China
6.Chinese Acad Sci, Xinjiang Astron Observ, 150, Sci-1 St, Urumqi 830011, Xinjiang, Peoples R China
7.Yuncheng Univ, Dept Phys & Elect Engn, Yuncheng 044000, Shanxi, Peoples R China
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GB/T 7714
Chen, J. L.,Wen, Z. G.,Duan, X. F.,et al. Individual pulse emission from the diffuse drifter PSR J1401-6357 using the ultrawideband receiver on the Parkes radio telescope[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2023,519(2):2709-2717.
APA Chen, J. L..,Wen, Z. G..,Duan, X. F..,He, D. L..,Wang, N..,...&Cui, S. R..(2023).Individual pulse emission from the diffuse drifter PSR J1401-6357 using the ultrawideband receiver on the Parkes radio telescope.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,519(2),2709-2717.
MLA Chen, J. L.,et al."Individual pulse emission from the diffuse drifter PSR J1401-6357 using the ultrawideband receiver on the Parkes radio telescope".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 519.2(2023):2709-2717.

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