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The Timing and Polarization of PSR J0002+6216

文献类型：期刊论文

作者Wei, Y.1,2,3,7; Wang, N.1,2,3; Yuan, J. P.1,2,3; Yao, J. M.1,2,3; Ge, M. Y.4; Dang, S. J.5,6; Zhao, D.1,2,3; Kou, F. F.1,2,3; Liu, P.8; Bai, J. T.1,2,3
刊名ASTROPHYSICAL JOURNAL
出版日期2025-05-01
卷号984期号:1页码:64
ISSN号0004-637X
DOI10.3847/1538-4357/adc714
产权排序2
英文摘要The combined timing analysis of data from the Five-hundred-meter Aperture Spherical radio Telescope (FAST) and the Fermi Large Area Telescope confirmed that PSR J0002+6216 is not a hyper-velocity (exceeding 1000 km s-1) pulsar. From this analysis, we determined the total proper motion of PSR J0002+6216 to be mu tot = 39.05 +/- 15.79 mas yr-1, which is consistent with Very Long Baseline Interferometry (VLBI) measurements to within 0.24 sigma. Moreover, two glitches were detected for the first time, which occurred on MJD 58850(17) and MJD 60421(6), respectively. The second glitch exhibited an exponential recovery process, with Q = 0.0090(3) and tau d = 45(3) days. Additionally, with FAST high-sensitivity observations, we measured the interstellar rotation measure (RM) and the 3D orientation of the spin axis for the first time, and updated the dispersion measure (DM) of PSR J0002+6216. Currently, no variations in RM or DM have been detected. By combining the measured RM with the observed position angle of the spin axis, we determined that the intrinsic position angle of the pulsar's spin axis is psi 0(intrinsic)=89.degrees 9 +/- 4.degrees 6 . When we compared this with the proper motion position angle obtained from VLBI, we found a misalignment of approximately 23 degrees between the spin and velocity angles of PSR J0002+6216. At present, pulsars with 2D spin-velocity angle measurements are unable to fully test the Janka et al. model. However, with more high-precision observational data in the future, we will be able to further test models related to pulsar birth.
WOS关键词SPIN-VELOCITY ALIGNMENT ; VORTEX CREEP ; PULSAR ; GLITCHES ; ROTATION ; PACKAGE ; ASTROMETRY ; DISCOVERY ; SOFTWARE ; TEMPO2
资助项目The National Science Foundation of Xinjiang Uygur Autonomous Region[2022D01D85] ; National Science Foundation of Xinjiang Uygur Autonomous Region[12288102] ; National Natural Science Foundation of China[YSBR-063] ; CAS Project for Young Scientists in Basic Research[2022-XBQNXZ-015] ; CAS Project for Young Scientists in Basic Research[xbzg-zdsys-202410] ; Chinese Academy of Sciences (CAS) Light of West China Program[2022A03013-4] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[ZK[2022]304] ; Guizhou Provincial Science and Technology Foundation[[2022]132] ; Scientific Research Project of the Guizhou Provincial Education[(2020) 003] ; Foundation of Education Bureau of Guizhou Province, China
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001477991300001
出版者IOP Publishing Ltd
资助机构The National Science Foundation of Xinjiang Uygur Autonomous Region ; National Science Foundation of Xinjiang Uygur Autonomous Region ; National Natural Science Foundation of China ; CAS Project for Young Scientists in Basic Research ; Chinese Academy of Sciences (CAS) Light of West China Program ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Guizhou Provincial Science and Technology Foundation ; Scientific Research Project of the Guizhou Provincial Education ; Foundation of Education Bureau of Guizhou Province, China
源URL[http://ir.xao.ac.cn/handle/45760611-7/7711]  
专题脉冲星研究团组
通讯作者Wang, N.; Yao, J. M.
作者单位1.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
2.Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Xinjiang, Peoples R China
3.Xinjiang Key Lab Radio Astrophys, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
4.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
5.Guizhou Normal Univ, Guizhou Prov Key Lab Radio Astron & Data Proc, Guiyang 550001, Peoples R China
6.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550001, Peoples R China
7.Xinjiang Univ, Sch Phys Sci & Technol, Urumqi 830046, Xinjiang, Peoples R China
8.Xiamen Univ, Dept Astron, Xiamen 361005, Fujian, Peoples R China
推荐引用方式
GB/T 7714		 Wei, Y.,Wang, N.,Yuan, J. P.,et al. The Timing and Polarization of PSR J0002+6216[J]. ASTROPHYSICAL JOURNAL,2025,984(1):64.
APA Wei, Y..,Wang, N..,Yuan, J. P..,Yao, J. M..,Ge, M. Y..,...&Bai, J. T..(2025).The Timing and Polarization of PSR J0002+6216.ASTROPHYSICAL JOURNAL,984(1),64.
MLA Wei, Y.,et al."The Timing and Polarization of PSR J0002+6216".ASTROPHYSICAL JOURNAL 984.1(2025):64.

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