中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Reciprocating Magnetic Fields in the Pulsar Wind Observed from the Black Widow Pulsar J1720-0534

文献类型:期刊论文

作者Miao, Chen-Chen11,12; Blackmon, Victoria10; Zhu, Wei-Wei9,12; Li, Dong-Zi8; Ge, Ming-Yu7; You, Xiao-Peng6; Mclaughlin, Maura10; Li, Di5,12; Wang, Na4; Wang, Pei9,12
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2023-10-01
卷号23期号:10页码:105005
关键词(stars:) pulsars: general (stars:) binaries: eclipsing
ISSN号1674-4527
DOI10.1088/1674-4527/ace179
产权排序9
英文摘要We report the radio observations of the eclipsing black widow pulsar J1720-0534, a 3.26 ms pulsar in orbit with a low mass companion of mass 0.029 to 0.034 M & ODOT;. We obtain the phase-connected timing ephemeris and polarization profile of this millisecond pulsar (MSP) using the Five-hundred-meter Aperture Spherical radio Telescope (FAST), the Green Bank Telescope (GBT), and the Parkes Telescope. For the first time from such a system, an oscillatory polarization angle change was observed from a particular eclipse egress with partial depolarization, indicating 10-milliGauss-level reciprocating magnetic fields oscillating in a length scale of 5 x 103 km (assuming an orbital inclination angle of 90 & DEG;) outside the companion's magnetosphere. The dispersion measure variation observed during the ingresses and egresses shows the rapid raising of the electron density in the shock boundary between the companion's magnetosphere and the surrounding pulsar wind. We suggest that the observed oscillatory magnetic fields originate from the pulsar wind outside the companion's magnetosphere.
WOS关键词MILLISECOND PULSAR ; ROTATION ; ECLIPSE ; EVOLUTION ; SHOCK
资助项目Australian Government ; National Natural Science Foundation of China (NSFC)[12041303] ; National Natural Science Foundation of China (NSFC)[12041304] ; National Natural Science Foundation of China (NSFC)[11873067] ; National Natural Science Foundation of China (NSFC)[12133004] ; National Natural Science Foundation of China (NSFC)[12203045] ; National Natural Science Foundation of China (NSFC)[12203070] ; National Natural Science Foundation of China (NSFC)[12203072] ; National Natural Science Foundation of China (NSFC)[12103013] ; National Natural Science Foundation of China (NSFC)[U2031117] ; National Natural Science Foundation of China (NSFC)[T2241020] ; CAS-MPG LEGACY project ; National SKA Program of China[2020SKA0120200] ; Foundation of Science and Technology of Guizhou Province[(2021)023] ; Foundation of Guizhou Provincial Education Department[KY(2021)303] ; National Key Research and Development Program of China[2022YFC2205202] ; National Key Research and Development Program of China[2022YFC2205203] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-1] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-3] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-4] ; 2021 project Xinjiang Uygur autonomous region of China for Tianshan elites ; Youth Innovation Promotion Association of CAS[2023069] ; Youth Innovation Promotion Association CAS[2021055] ; CAS Project for Young Scientists in Basic Research[YSBR-006] ; Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS ; Zhejiang Provincial Natural Science Foundation of China[LY23A030001] ; NSF Physics Frontiers Center award[2020265]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001067094200001
出版者NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
资助机构Australian Government ; National Natural Science Foundation of China (NSFC) ; CAS-MPG LEGACY project ; National SKA Program of China ; Foundation of Science and Technology of Guizhou Province ; Foundation of Guizhou Provincial Education Department ; National Key Research and Development Program of China ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; 2021 project Xinjiang Uygur autonomous region of China for Tianshan elites ; Youth Innovation Promotion Association of CAS ; Youth Innovation Promotion Association CAS ; CAS Project for Young Scientists in Basic Research ; Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CAS ; Zhejiang Provincial Natural Science Foundation of China ; NSF Physics Frontiers Center award
源URL[http://ir.xao.ac.cn/handle/45760611-7/5532]  
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Miao, Chen-Chen
作者单位1.Cent China Normal Univ, Coll Phys Sci & Technol, Wuhan 430079, Peoples R China
2.Fudan Univ, Sch Comp Sci, Shanghai 200433, Peoples R China
3.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
4.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
5.Res Ctr Intelligent Comp Platforms, Zhejiang Lab, Hangzhou 311100, Peoples R China
6.Southwest Univ, Sch Phys Sci & Technol, Chongqing 400715, Peoples R China
7.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
8.CALTECH, Cahill Ctr Astron & Astrophys, 1216 Calif Blvd, Pasadena, CA 91125 USA
9.Beijing Normal Univ, Inst Frontiers Astron & Astrophys, Beijing 102206, Peoples R China
10.West Virginia Univ, 1500 Univ Ave, Morgantown, WV 26506 USA
推荐引用方式
GB/T 7714
Miao, Chen-Chen,Blackmon, Victoria,Zhu, Wei-Wei,et al. Reciprocating Magnetic Fields in the Pulsar Wind Observed from the Black Widow Pulsar J1720-0534[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2023,23(10):105005.
APA Miao, Chen-Chen.,Blackmon, Victoria.,Zhu, Wei-Wei.,Li, Dong-Zi.,Ge, Ming-Yu.,...&Zhao, De.(2023).Reciprocating Magnetic Fields in the Pulsar Wind Observed from the Black Widow Pulsar J1720-0534.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,23(10),105005.
MLA Miao, Chen-Chen,et al."Reciprocating Magnetic Fields in the Pulsar Wind Observed from the Black Widow Pulsar J1720-0534".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 23.10(2023):105005.

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