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The Single-pulse Observation of PSR B2111+46 with the Five-hundred-meter Aperture Spherical Radio Telescope
Zhi, Q. J.1,2; Bai, J. T.2,3,4; Shang, L. H.1,2; Xu, X.2,5; Dang, S. J.1,2; Li, D.6,7,8; Zhang, L.6; Wang, P.6; Xie, X. Y.9; Zhao, R. S.1,2; Dong, A. J.1,2; Qiao, G. J.10
2023-09-01
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume954Issue:1Pages:24
Contribution Rank3
AbstractWe report the observations of periodic nulling in PSR B2111+46 at 1250 MHz with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The nulling fractions (NF) as well as nulling period of this pulsar were calculated. The NF and nulling period are 17% & PLUSMN; 1% and 62.49 & PLUSMN; 0.99 P (1), respectively, and the periodic nulling shows variations in periodicity with time. The durations of each consecutive burst and nulling were investigated, which show that the power-law distribution and the indices are -1.11 & PLUSMN; 0.04 and -2.08 & PLUSMN; 0.23. In the observed frequency band, the width of the profile is narrowed with the increase in frequency, and the degree of polarization has no obvious trend with the increase in frequency. We discovered a weak emission component in front of the leading component of this triple-type profile pulsar that was not observed in other bands and by other telescopes. With the fitting of rotation vector model, we obtained that the angles of the magnetic inclination & alpha; and the line of sight & zeta; are & SIM;13.& DEG;0 and & SIM;11.& DEG;6, respectively. The high-sensitivity observation of FAST improves our understanding of the emission of this pulsar.
DOI10.3847/1538-4357/ace362
Indexed BySCI
Language英语
WOS KeywordINVERSE COMPTON-SCATTERING ; MULTICOMPONENT GAUSSIAN FITS ; GEOMETRICAL ANALYSIS ; EMISSION ; MODEL ; POLARIZATION ; PROFILES ; NULLS ; POLARIMETRY ; FREQUENCIES
Funding ProjectNational Natural Science Foundation ; National Natural Science Foundation[12273008] ; National Natural Science Foundation[11988101] ; National Natural Science Foundation[U1731238] ; National Natural Science Foundation[U1831120] ; National Natural Science Foundation[U1838106] ; National Natural Science Foundation[61875087] ; National Natural Science Foundation[61803373] ; National Natural Science Foundation[11303069] ; National Natural Science Foundation[11373011] ; National Natural Science Foundation[11873080] ; National Natural Science Foundation[U2031117] ; National Natural Science Foundation[12041304] ; National Natural Science Foundation[12288102] ; National Key Ramp ; D Program of China[2017YFB0503300] ; National SKA Program of China[2022SKA0130100] ; National SKA Program of China[2022SKA0130104] ; Guizhou Provincial Science and Technology Foundation[ZK[2023]024] ; Guizhou Provincial Science and Technology Foundation[ZK[2022]304] ; Guizhou Provincial Science and Technology Foundation[[2016]4008] ; Guizhou Provincial Science and Technology Foundation[[2017]5726-37] ; Guizhou Provincial Science and Technology Foundation[[2018]5769-02] ; Foundation of Guizhou Provincial Education Department[KY (2020) 003)] ; Scientific Research Project of the Guizhou Provincial Education[KY[2022]137] ; Scientific Research Project of the Guizhou Provincial Education[KY[2022]123] ; Scientific Research Project of the Guizhou Provincial Education[KY[2022]132] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-4] ; Youth Innovation Promotion Association CAS[2021055] ; CAS Project for Young Scientists in Basic Reasearch[YSBR-006] ; Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001051655500001
PublisherIOP Publishing Ltd
Funding OrganizationNational Natural Science Foundation ; National Natural Science Foundation ; National Key Ramp ; D Program of China ; National SKA Program of China ; Guizhou Provincial Science and Technology Foundation ; Foundation of Guizhou Provincial Education Department ; Scientific Research Project of the Guizhou Provincial Education ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Youth Innovation Promotion Association CAS ; CAS Project for Young Scientists in Basic Reasearch ; Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS
Citation statistics
Cited Times:6[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/5390
Collection中国科学院新疆天文台
射电天文研究室_脉冲星研究团组
Corresponding AuthorZhi, Q. J.
Affiliation1.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550001, Peoples R China
2.Guizhou Normal Univ, Guizhou Prov Key Lab Radio Astron & Data Proc, Guiyang 550001, Peoples R China
3.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
4.Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China
5.Guizhou Normal Univ, Sch Math Sci, Guiyang 550001, Peoples R China
6.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
7.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
8.Univ KwaZulu Natal, NAOC UKZN Computat Astrophys Ctr, ZA-4000 Durban, South Africa
9.Guizhou Normal Univ, Key Lab Informat & Comp Sci Guizhou Prov, Guiyang 550001, Peoples R China
10.Peking Univ, Sch Phys, Beijing 100871, Peoples R China
Recommended Citation
GB/T 7714
Zhi, Q. J.,Bai, J. T.,Shang, L. H.,et al. The Single-pulse Observation of PSR B2111+46 with the Five-hundred-meter Aperture Spherical Radio Telescope[J]. ASTROPHYSICAL JOURNAL,2023,954(1):24.
APA Zhi, Q. J..,Bai, J. T..,Shang, L. H..,Xu, X..,Dang, S. J..,...&Qiao, G. J..(2023).The Single-pulse Observation of PSR B2111+46 with the Five-hundred-meter Aperture Spherical Radio Telescope.ASTROPHYSICAL JOURNAL,954(1),24.
MLA Zhi, Q. J.,et al."The Single-pulse Observation of PSR B2111+46 with the Five-hundred-meter Aperture Spherical Radio Telescope".ASTROPHYSICAL JOURNAL 954.1(2023):24.
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