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High-altitude Magnetospheric Emissions from Two Pulsars
Yuan, Mao1,2; Zhu, Weiwei1; Kramer, Michael3; Peng, Bo1; Lu, Jiguang1; Xu, Renxin4,5; Shao, Lijing5; Wang, Hong-Guang6; Meng, Lingqi1,2; Niu, Jiarui1,2; Zhao, Rushuang1; Miao, Chenchen1,2; Miao, Xueli1; Xue, Mengyao1; Feng, Yi7; Wang, Pei1; Li, Di1; Zhang, Chengming1; Champion, David J.3; Fonseca, Emmanuel8,9; Hu, Huanchen3; Yao, Jumei10; Freire, Paulo C. C.3; Guo, Yanjun3
2023-06-01
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume949Issue:2Pages:115
Contribution Rank10
AbstractWe discover three new weak pulse components in two known pulsars, one in PSR J0304+1932 and two in PSR J1518+4904. These components are emitted about halfway between the main emission beam and the interpulse beam (beam from the opposite pole). They are separated from their main pulse peak by 99 degrees +/- 3 degrees for J0304+1932 and 123.degrees 6 +/- 0.degrees 7 (leading) and 93 degrees +/- 0.degrees 4 (trailing) for J1518+4904. Their peak-intensity ratios to main pulses are similar to 0.06% for J0304+1932 and similar to 0.17% and similar to 0.83% for J1518+4904. We also analyzed the flux fluctuations and profile variations of the emissions for the two pulsars. The results show correlations between the weak pulses and their main pulses, indicating that these emissions come from the same pole. We estimated the emission altitude of these weak pulses and derived a height of about half of the pulsar's light-cylinder radius. These pulse components are a unique sample of high-altitude emissions from pulsars, and challenge the current pulsar emission models.
DOI10.3847/1538-4357/accb9a
Indexed BySCI
Language英语
WOS KeywordRADIO-EMISSION ; EMPIRICAL-THEORY ; FREQUENCY-DEPENDENCE ; INTEGRATED PROFILES ; CORE EMISSION ; MAIN PULSE ; X-RAY ; MODE ; POLARIZATION ; GEOMETRY
Funding ProjectChinese Academy of Sciences - National SKA Program of China ; National Nature Science Foundation[12003028] ; National Nature Science Foundation[2020SKA0120200] ; National Nature Science Foundation[2020SKA0120100] ; National Nature Science Foundation[2020SKA0120300] ; MPG-CAS LEGAC collaboration ; National Astronomical Observatories, Chinese Academy of Sciences ; National SKA Program of China ; [12041303] ; [11873067] ; [12041304]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001000805600001
PublisherIOP Publishing Ltd
Funding OrganizationChinese Academy of Sciences - National SKA Program of China ; National Nature Science Foundation ; MPG-CAS LEGAC collaboration ; National Astronomical Observatories, Chinese Academy of Sciences ; National SKA Program of China
Citation statistics
Cited Times:5[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/5496
Collection射电天文研究室_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
Corresponding AuthorYuan, Mao
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
2.Univ Chinese Acad Sci, Coll Astron & Space Sci, Beijing 100049, Peoples R China
3.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
4.Peking Univ, Dept Astron, Beijing 100871, Peoples R China
5.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
6.Guangzhou Univ, Dept Astron, Guangzhou 510006, Peoples R China
7.Zhejiang Lab, Res Inst Artificial Intelligence, Hangzhou 311121, Zhejiang, Peoples R China
8.West Virginia Univ, Dept Phys & Astron, POB 6315, Morgantown, WV 26506 USA
9.West Virginia Univ, Ctr Gravitat Waves & Cosmol, Chestnut Ridge Res Bldg, Morgantown, WV 26505 USA
10.Chinese Acad Sci, Xinjiang Astron Observ, 150,Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
Recommended Citation
GB/T 7714
Yuan, Mao,Zhu, Weiwei,Kramer, Michael,et al. High-altitude Magnetospheric Emissions from Two Pulsars[J]. ASTROPHYSICAL JOURNAL,2023,949(2):115.
APA Yuan, Mao.,Zhu, Weiwei.,Kramer, Michael.,Peng, Bo.,Lu, Jiguang.,...&Guo, Yanjun.(2023).High-altitude Magnetospheric Emissions from Two Pulsars.ASTROPHYSICAL JOURNAL,949(2),115.
MLA Yuan, Mao,et al."High-altitude Magnetospheric Emissions from Two Pulsars".ASTROPHYSICAL JOURNAL 949.2(2023):115.
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