中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Change of Rotation Measure during the Eclipse of a Black Widow PSR J2051-0827

文献类型:期刊论文

作者Wang, S. Q.12,13,14; Wang, J. B.11; Li, D. Z.10; Yao, J. M.12,13,14; Manchester, R. N.9; Hobbs, G.9; Wang, N.12,13,14; Dai, S.8; Xu, H.7; Luo, R.6,9
刊名ASTROPHYSICAL JOURNAL
出版日期2023-09-01
卷号955期号:1页码:6
ISSN号0004-637X
DOI10.3847/1538-4357/acea81
通讯作者Wang, S. Q.(wangshuangqiang@xao.ac.cn)
英文摘要Black widows are millisecond pulsars ablating their companions. The material blown from the companion blocks the radio emission, resulting in radio eclipses. The properties of the eclipse medium are poorly understood. Here, we present direct evidence of the existence of magnetic fields in the eclipse medium of the black widow PSR J2051-0827 using observations made with the Five-hundred-meter Aperture Spherical radio Telescope. We detect a regular decrease in rotation measure (RM) in the egress of the eclipse, changing from 60 to -28.7 rad m-2. The RM gradually changes back to normal when the line of sight moves away from the eclipse. The estimated line-of-sight magnetic field strength in the eclipse medium is & SIM;0.1 G. The RM reversal could be caused by a change in the magnetic field strength along the line of sight due to binary orbital motion. The RM reversal phenomenon has also been observed in some repeating fast radio bursts (FRBs), and the study of spider pulsars may provide additional information about the origin of FRBs.
WOS关键词RADIO-BURST SOURCE ; MILLISECOND PULSAR ; MAGNETIC-FIELDS ; BINARY PULSAR ; POLARIZATION ; ENVIRONMENT ; COMPANION ; DECADE ; STAR
资助项目National Key Research and Development Program of China[2022YFC2205202] ; National Key Research and Development Program of China[2021YFC2203502] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-3] ; National Natural Science Foundation of China[12288102] ; National Natural Science Foundation of China[12203092] ; National Natural Science Foundation of China[12041304] ; National Natural Science Foundation of China[U1938117] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[2022D01B71] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[2022D01D85] ; CAS ; National SKA Program of China[2020SKA0120100] ; CAS Project for Young Scientists in Basic Research[YSBR-063] ; Key Research Project of Zhejiang Laboratory[2021PE0AC03] ; Zhejiang Provincial Natural Science Foundation of China[LY23A030001] ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP Publishing Ltd
WOS记录号WOS:001065942500001
资助机构National Key Research and Development Program of China ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; National Natural Science Foundation of China ; Natural Science Foundation of Xinjiang Uygur Autonomous Region ; CAS ; National SKA Program of China ; CAS Project for Young Scientists in Basic Research ; Key Research Project of Zhejiang Laboratory ; Zhejiang Provincial Natural Science Foundation of China ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments
源URL[http://ir.xao.ac.cn/handle/45760611-7/5454]  
专题研究单元未命名
通讯作者Wang, S. Q.
作者单位1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
2.Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China
3.Univ KwaZulu Natal, NAOC UKZN Computat Astrophys Ctr, ZA-4000 Durban, South Africa
4.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
5.Zhejiang Lab, Hangzhou 311121, Zhejiang, Peoples R China
6.Guangzhou Univ, Sch Phys & Mat Sci, Dept Astron, Guangzhou 510006, Peoples R China
7.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
8.Western Sydney Univ, Sch Sci, Penrith, NSW 2751, Australia
9.CSIRO Space & Astron, POB 76, Epping, NSW 1710, Australia
10.CALTECH, Cahill Ctr Astron & Astrophys, 1216 E Calif Blvd, Pasadena, CA 91125 USA
推荐引用方式
GB/T 7714
Wang, S. Q.,Wang, J. B.,Li, D. Z.,et al. Change of Rotation Measure during the Eclipse of a Black Widow PSR J2051-0827[J]. ASTROPHYSICAL JOURNAL,2023,955(1):6.
APA Wang, S. Q..,Wang, J. B..,Li, D. Z..,Yao, J. M..,Manchester, R. N..,...&Zhang, C. M..(2023).Change of Rotation Measure during the Eclipse of a Black Widow PSR J2051-0827.ASTROPHYSICAL JOURNAL,955(1),6.
MLA Wang, S. Q.,et al."Change of Rotation Measure during the Eclipse of a Black Widow PSR J2051-0827".ASTROPHYSICAL JOURNAL 955.1(2023):6.

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