中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Exploring the Individual Pulse Behavior of Pulsar J1701-3726 with Parkes

文献类型:期刊论文

作者Wang, H.8; Wen, Z. G.7; Duan, X. F.6,7; Wang, Z.5,7; He, D. L.7; Wang, H. G.4,7; Wang, N.7; Yuan, J. P.7; Yan, W. M.7; Yuen, R.7
刊名ASTROPHYSICAL JOURNAL
出版日期2023-06-01
卷号950期号:2页码:11
ISSN号0004-637X
DOI10.3847/1538-4357/acd17b
通讯作者Wen, Z. G.(wenzhigang@xao.ac.cn)
英文摘要We have carried out a detailed study of polarimetric individual pulse emission from the pulsar J1701-3726 (B1658-37), observed at 1369 MHz using the Parkes 64 m radio telescope. The single-pulse sequences reveal the presence of the three major emission phenomena of pulse nulling, mode changing, and subpulse drifting. Trimodal distribution of the pulse energy is present, implying one population of nulls and two others of emission in the phase window. The mean flux density of the normal mode is almost two times that of the abnormal mode. Our data show that, for PSR J1701-3726, 64% of the time was spent in the normal mode and 12% was in the abnormal mode. The single pulses show the presence of two distinct periodic modulations using a fluctuation spectral analysis. About 24% of the nulls are found to create alternating bunches of nulls and bursts in a quasiperiodic manner with a longer periodicity of 48 & PLUSMN; 4 rotational periods. Additionally, the pulsar presents a steady even-odd modulated feature with a stationary longitude within the pulse window. The ramifications for constraining the viewing geometry and understanding the radio emission mechanisms are discussed.
WOS关键词NONRADIAL OSCILLATION MODEL ; DRIFTING SUBPULSES ; FLUCTUATION SPECTRA ; RADIO PULSAR ; EMISSION ; MODULATION ; PROFILES ; GEOMETRY ; MECHANISM ; NULLS
资助项目Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-1] ; National Key Research and Development Program of China[2022YFC2205203] ; Chinese Academy of Sciences Foundation of the young scholars of western[2020-XBQNXZ-019] ; open project of the Key Laboratory in Xinjiang Uygur Autonomous Region of China[2023D04058] ; National Natural Science Foundation of China (NSFC)[11988101] ; National Natural Science Foundation of China (NSFC)[U1838109] ; National Natural Science Foundation of China (NSFC)[12041304] ; National Natural Science Foundation of China (NSFC)[12041301] ; National Natural Science Foundation of China (NSFC)[11873080] ; National Natural Science Foundation of China (NSFC)[12133004] ; National Natural Science Foundation of China (NSFC)[12203094] ; National Natural Science Foundation of China (NSFC)[U1631106] ; National SKA Program of China[2020SKA0120100] ; Youth Innovation Promotion Association of CAS[2023069] ; Natural Science Foundation of Shanxi Province[20210302123083] ; Scientific and Technological Innovation Programs of Higher Education Institutions in Shanxi[2021L480] ; Yucheng University[YQ-20211027] ; 2021 project Xinjiang Uygur autonomous region of China ; CAS Jianzhihua project ; 2018 project of Xinjiang Uygur autonomous region of China ; CAS Light of West China Program[2019-XBQNXZ-B-019] ; Australian Government
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001012790600001
出版者IOP Publishing Ltd
资助机构Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; National Key Research and Development Program of China ; Chinese Academy of Sciences Foundation of the young scholars of western ; open project of the Key Laboratory in Xinjiang Uygur Autonomous Region of China ; National Natural Science Foundation of China (NSFC) ; National SKA Program of China ; Youth Innovation Promotion Association of CAS ; Natural Science Foundation of Shanxi Province ; Scientific and Technological Innovation Programs of Higher Education Institutions in Shanxi ; Yucheng University ; 2021 project Xinjiang Uygur autonomous region of China ; CAS Jianzhihua project ; 2018 project of Xinjiang Uygur autonomous region of China ; CAS Light of West China Program ; Australian Government
源URL[http://ir.xao.ac.cn/handle/45760611-7/5274]  
专题研究单元未命名
通讯作者Wen, Z. G.
作者单位1.Jihua Lab, Foshan 528200, Guangdong, Peoples R China
2.Xinjiang Univ, Sch Mech Engn, Urumqi 830017, Xinjiang, Peoples R China
3.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550001, Guizhou, Peoples R China
4.Guangzhou Univ, Sch Phys & Elect Engn, Guangzhou 510006, Peoples R China
5.Xinjiang Key Lab Radio Astrophys, Urumqi 830011, Xinjiang, Peoples R China
6.Key Lab Microwave Technol, Urumqi 830011, Xinjiang, Peoples R China
7.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
8.Yuncheng Univ, Dept Phys & Elect Engn, Yuncheng 044000, Shanxi, Peoples R China
推荐引用方式
GB/T 7714
Wang, H.,Wen, Z. G.,Duan, X. F.,et al. Exploring the Individual Pulse Behavior of Pulsar J1701-3726 with Parkes[J]. ASTROPHYSICAL JOURNAL,2023,950(2):11.
APA Wang, H..,Wen, Z. G..,Duan, X. F..,Wang, Z..,He, D. L..,...&Ergesh, T..(2023).Exploring the Individual Pulse Behavior of Pulsar J1701-3726 with Parkes.ASTROPHYSICAL JOURNAL,950(2),11.
MLA Wang, H.,et al."Exploring the Individual Pulse Behavior of Pulsar J1701-3726 with Parkes".ASTROPHYSICAL JOURNAL 950.2(2023):11.

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