The Single-pulse Observation of PSR B2111+46 with the Five-hundred-meter Aperture Spherical Radio Telescope
文献类型：期刊论文
| 作者 | Zhi, Q. J.9,10; Bai, J. T.7,8,9; Shang, L. H.9,10; Xu, X.6,9; Dang, S. J.9,10; Li, D.3,4,5; Zhang, L.5 ; Wang, P.5; Xie, X. Y.2; Zhao, R. S.9,10
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| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2023-09-01 |
| 卷号 | 954期号:1页码:11 |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/ace362 |
| 通讯作者 | Zhi, Q. J.(qjzhi@gznu.edu.cn) |
| 英文摘要 | We 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. |
| WOS关键词 | INVERSE COMPTON-SCATTERING ; MULTICOMPONENT GAUSSIAN FITS ; GEOMETRICAL ANALYSIS ; EMISSION ; MODEL ; POLARIZATION ; PROFILES ; NULLS ; POLARIMETRY ; FREQUENCIES |
| 资助项目 | National 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研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:001051655500001 |
| 出版者 | IOP Publishing Ltd |
| 资助机构 | National 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 |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/5389]  |
| 专题 | 研究单元未命名 |
| 通讯作者 | Zhi, Q. J. |
| 作者单位 | 1.Peking Univ, Sch Phys, Beijing 100871, Peoples R China 2.Guizhou Normal Univ, Key Lab Informat & Comp Sci Guizhou Prov, Guiyang 550001, Peoples R China 3.Univ KwaZulu Natal, NAOC UKZN Computat Astrophys Ctr, ZA-4000 Durban, South Africa 4.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 5.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China 6.Guizhou Normal Univ, Sch Math Sci, Guiyang 550001, Peoples R China 7.Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China 8.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 9.Guizhou Normal Univ, Guizhou Prov Key Lab Radio Astron & Data Proc, Guiyang 550001, Peoples R China 10.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550001, Peoples R China |
| 推荐引用方式 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):11. |
| 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),11. |
| 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):11. |
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