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Single-pulse Emissions of PSRs J1611-0114 and J1617+1123
Liu, Shifang1,2; Wen, Zhigang2,3,4; Wang, Shuangqiang2,3; Kou, Feifei2,4; Yan, Wenming2,3,4; Yuan, Jianping1,2,3; Wu, Qingdong2,3; Zhao, De1,2; Miao, Chenchen5; Wang, Na1,2,3; Xue, Menyao5; Li, Di5,6; Wang, Pei5; Sun, Shengnan2; Zhu, Weiwei5; Bai, Juntao2,3
2024-11-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
ISSN1674-4527
Volume24Issue:11Pages:115001
Contribution Rank2
AbstractIn this paper, the emissions from two pulsars, PSRs J1611-0114 and J1617+1123, were investigated using the Five-hundred-meter Aperture Spherical radio Telescope operating at a central frequency of 1250 MHz. The average pulse profile of PSR J1611-0114 shows two components, the first of which is relatively weak in intensity. The two-dimensional pulse stack exhibits an obvious nulling phenomenon, with an estimated nulling fraction of 40.1% +/- 5.4%. The durations of the nulls and bursts are consistent with power-law distributions, and no periodic nulling phenomenon is found. The results from PSR J1617+1123 demonstrate that the average pulse profile is composed of four components. The peak intensity of the fourth component varies significantly, causing an unstable integrated profile. In addition, the modulation characteristics of J1611-0114 and J1617+1123 were studied by analyzing the modulation index, longitude resolved fluctuation spectrum and two-dimensional fluctuation spectrum using the software PSRSALSA. It was found that the two pulsars exhibit intensity modulation. In particular, J1611-0114 displays even-odd modulation, with the modulation period of approximately two pulses. The modulation period of J1617+1123 is relatively broad. There is an obvious subpulse drift phenomenon, and the value of P-2 is similar to 0.125c/P (0), corresponding to 12 pulse longitude bins, and the drift rate (P-2/P-3) is about 0.29.
Keywordstars: neutron ( stars: ) pulsars: general stars: neutron ( stars: ) pulsars: individual ( PSRs J1611-0114-0114 and J1617+1123)+1123 )
DOI10.1088/1674-4527/ad7fb6
Indexed BySCI
Language英语
WOS KeywordSUBPULSE MODULATION ; BEHAVIOR
Funding ProjectNational Key Research and Development Program of China[2022YFC2205203] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-4] ; National Natural Science Foundation of China (NSFC)[12041303] ; National Natural Science Foundation of China (NSFC)[12273100] ; National Natural Science Foundation of China (NSFC)[12288102] ; Youth Innovation Promotion Association of CAS[2023069] ; Tianshan Talent Training Program[2023TSYCCX0100] ; National SKA Program of China[2020SKA0120200] ; National Key R&D Program of China[2022YFC2205201] ; West Light Foundation of the Chinese Academy of Sciences ; WLFC[2021-XBQNXZ-027]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001337707400001
PublisherNATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
Funding OrganizationNational Key Research and Development Program of China ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; National Natural Science Foundation of China (NSFC) ; Youth Innovation Promotion Association of CAS ; Tianshan Talent Training Program ; National SKA Program of China ; National Key R&D Program of China ; West Light Foundation of the Chinese Academy of Sciences ; WLFC
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Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/7075
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, Jianping
Affiliation1.Xinjiang Univ, Sch Phys & Technol, Urumqi 830046, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830046, Peoples R China
3.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
4.Xinjiang Key Lab Radio Astrophys, Urumqi 830046, Peoples R China
5.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
6.Tsinghua Univ, Dept Astron, Beijing 100084, Peoples R China
Recommended Citation
GB/T 7714
Liu, Shifang,Wen, Zhigang,Wang, Shuangqiang,et al. Single-pulse Emissions of PSRs J1611-0114 and J1617+1123[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2024,24(11):115001.
APA Liu, Shifang.,Wen, Zhigang.,Wang, Shuangqiang.,Kou, Feifei.,Yan, Wenming.,...&Bai, Juntao.(2024).Single-pulse Emissions of PSRs J1611-0114 and J1617+1123.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,24(11),115001.
MLA Liu, Shifang,et al."Single-pulse Emissions of PSRs J1611-0114 and J1617+1123".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 24.11(2024):115001.
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