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Timing and Scintillation Studies of Pulsars in Globular Cluster M3 (NGC 5272) with FAST

文献类型：期刊论文

作者Li, Baoda15,16; Zhang, Li-yun15,16; Yao, Jumei1,2,8; Yin, Dejiang16; Eatough, Ralph P.6,7; Li, Minghui5; Li, Yifeng3,4; Lian, Yujie13,14; Pan, Yu12; Dai, Yinfeng16
刊名ASTROPHYSICAL JOURNAL
出版日期2024-09-01
卷号972期号:1页码:43
ISSN号0004-637X
DOI10.3847/1538-4357/ad5a82
产权排序3
英文摘要We present the phase-connected timing solutions of all five pulsars in globular cluster M3 (NGC 5272), namely PSRs M3A to F (PSRs J1342+2822A to F), with the exception of PSR M3C, from FAST archival data. In these timing solutions, those of PSRs M3E and F are obtained for the first time. We find that PSRs M3E and F have low-mass companions and are in circular orbits with periods of 7.1 and 3.0 days, respectively. For PSR M3C, we have not detected its signal in all 41 observations. We found no X-ray counterparts for these pulsars in archival Chandra images in the band of 0.2-20 keV. From the autocorrelation function analysis of M3A and M3B's dynamic spectra, the scintillation timescale ranges from 7.0 +/- 0.3 to 60.0 +/- 0.6 minutes, and the scintillation bandwidth ranges from 4.6 +/- 0.2 to 57.1 +/- 1.1 MHz. The measured scintillation bandwidths from the dynamic spectra indicate strong scintillation, and the scattering medium is anisotropic. From the secondary spectra, we captured a scintillation arc only for PSR M3B with a curvature of 649 +/- 23 m-1 mHz-2.
WOS关键词BINARY MILLISECOND PULSARS ; LONG-TERM SCINTILLATION ; DISCOVERY ; SCATTERING
资助项目National Key R&D Program of China[2022YFC2205202] ; National Key R&D Program of China[2020SKA0120100] ; National Natural Science Foundation of China[11703047] ; National Natural Science Foundation of China[11773041] ; National Natural Science Foundation of China[U2031119] ; National Natural Science Foundation of China[12173052] ; National Natural Science Foundation of China[12173053] ; National Natural Science Foundation of China[12373032] ; National Natural Science Foundation of China[11963002] ; National Natural Science Foundation of China[12041304] ; National Natural Science Foundation of China[12041303] ; National Natural Science Foundation of China[12288102] ; National Science Foundation of Xinjiang Uygur Autonomous Region[2022D01D85] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-2] ; Tianchi Talent project[2023TSYCTD0013] ; CAS Project for Young Scientists in Basic Research[YSBR-063] ; CAS Light of West China Program ; Youth Innovation Promotion Association of the Chinese Academy of Sciences[2023064] ; Youth Innovation Promotion Association of the Chinese Academy of Sciences[2018075] ; Youth Innovation Promotion Association of the Chinese Academy of Sciences[Y2022027] ; Chinese Academy of Sciences President's International Fellowship Initiative[2021FSM0004] ; International Centre of Supernovae, Yunnan Key Laboratory[202302AN360001] ; International Centre of Supernovae, Yunnan Key Laboratory[202302AN36000104]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001296624800001
出版者IOP Publishing Ltd
资助机构National Key R&D Program of China ; National Natural Science Foundation of China ; National Science Foundation of Xinjiang Uygur Autonomous Region ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Tianchi Talent project ; CAS Project for Young Scientists in Basic Research ; CAS Light of West China Program ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Chinese Academy of Sciences President's International Fellowship Initiative ; International Centre of Supernovae, Yunnan Key Laboratory
源URL[http://ir.xao.ac.cn/handle/45760611-7/6928]  
专题脉冲星研究团组
科研仪器设备产出_我台利用FAST观测数据文章
通讯作者Zhang, Li-yun; Yao, Jumei; Qian, Lei; Pan, Zhichen
作者单位1.Chinese Acad Sci, Xinjiang Astron Observ, 150,Sci 1 St, Urumqi 550001, Xinjiang, Peoples R China
2.Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Xinjiang, Peoples R China
3.Chinese Acad Sci, Key Lab Time Reference & Applicat, Xian 710600, Peoples R China
4.Chinese Acad Sci, Natl Time Serv Ctr, Xian 710600, Peoples R China
5.Guizhou Univ, Guizhou, Peoples R China
6.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
7.Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100101, Peoples R China
8.Xinjiang Key Lab Radio Astrophys, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
9.Guizhou Univ, Guizhou Radio Astron Observ, Guiyang 550025, Peoples R China
10.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
推荐引用方式
GB/T 7714		 Li, Baoda,Zhang, Li-yun,Yao, Jumei,et al. Timing and Scintillation Studies of Pulsars in Globular Cluster M3 (NGC 5272) with FAST[J]. ASTROPHYSICAL JOURNAL,2024,972(1):43.
APA Li, Baoda.,Zhang, Li-yun.,Yao, Jumei.,Yin, Dejiang.,Eatough, Ralph P..,...&Pan, Zhichen.(2024).Timing and Scintillation Studies of Pulsars in Globular Cluster M3 (NGC 5272) with FAST.ASTROPHYSICAL JOURNAL,972(1),43.
MLA Li, Baoda,et al."Timing and Scintillation Studies of Pulsars in Globular Cluster M3 (NGC 5272) with FAST".ASTROPHYSICAL JOURNAL 972.1(2024):43.

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