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Single-pulse Emission Variation of Two Pulsars Discovered by FAST
Guo, Ziping1,2; Wen, Zhigang1,2,3; Yuan, Jianping1,2,3; Kou, Feifei1,2; Wu, Qingdong1,2; Wang, Na1,2,3; Zhu, Weiwei4; Li, Di2,4,7; Xue, Mengyao4; Wang, Pei4,8; Miao, Chenchen4; Zhao, De1,2; Hu, Yue5; Yan, Wenming1,2,3; Niu, Jiarui4; Rejep, Rukiye4; Huang, Zhipeng6
2023-07-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
ISSN1674-4527
Volume23Issue:7Pages:075008
Contribution Rank1
AbstractWe investigate the single-pulse emission variations of two pulsars, PSRs J0211+4235 and J0553+4111, observed with the Five-hundred-meter Aperture Spherical radio Telescope at the 1.25 GHz central frequency. The observation sessions span from 2020 December to 2021 July, with 21 and 22 observations for them respectively. The integrated pulse profile of PSR J0211+4235 shows that there is a weak pulse component following the main component, and PSR J0553+4111 displays a bimodal profile with a bridge component in the middle. PSR J0211+4235 presents significant nulling phenomenon with nulling duration lasting from 2 to 115 pulses and burst duration lasting from 2 to 113 pulses. The NF of each observation is determined to be 45%-55%. No emission greater than three s is found in the mean integrated profile of all nulling pulses. In most cases, the pulse energy changes abruptly during the transition from null to burst, while in the transition from burst to null there are two trends: abrupt and gradual. We find that the nulling phenomenon of PSR J0211+4235 is periodic by the Fourier transform of the null and burst state. In addition, the single-pulse modulation characteristics of these two pulsars are investigated, and the distributions of modulation index, LRFS and 2DFS are analyzed with PSRSALSA. The left peak of PSR J0553+4111 has intensity modulation. Finally, the polarization properties of these two pulsars are obtained through polarization calibration, and their characteristics are analyzed. The possible physical mechanisms of these phenomena are discussed.
Keyword(stars:) pulsars general - (stars:) pulsars individual (PSR J0211+4235, PSR J0553+4111) - stars neutron
DOI10.1088/1674-4527/accdc1
Indexed BySCI
Language英语
WOS KeywordEMPIRICAL-THEORY ; SUBPULSE MODULATION ; PERIODIC NULLS ; RADIO PULSARS ; PSR ; GEOMETRY ; MODES
Funding ProjectNational Key Research and Development Program of China[2022YFC2205203] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-1] ; National Natural Science Foundation of China (NSFC)[U1838109] ; National Natural Science Foundation of China (NSFC)[12041304] ; Youth Innovation Promotion Association of CAS[2023069] ; Natural Science Foundation of Shanghai[20ZR1467600] ; project Xinjiang Uygur autonomous region of China
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001015484700001
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 ; Natural Science Foundation of Shanghai ; project Xinjiang Uygur autonomous region of China
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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/45760611-7/5287
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.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
3.Xinjiang Key Lab Radio Astrophys, Urumqi 830011, Peoples R China
4.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
5.Chinese Acad Sci, Natl Time Serv Ctr NTSC, Xian 710600, Peoples R China
6.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
7.Zhejiang Lab, Hangzhou 311121, Peoples R China
8.Beijing Normal Univ, Inst Frontiers Astron & Astrophys, Beijing 102206, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Guo, Ziping,Wen, Zhigang,Yuan, Jianping,et al. Single-pulse Emission Variation of Two Pulsars Discovered by FAST[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2023,23(7):075008.
APA Guo, Ziping.,Wen, Zhigang.,Yuan, Jianping.,Kou, Feifei.,Wu, Qingdong.,...&Huang, Zhipeng.(2023).Single-pulse Emission Variation of Two Pulsars Discovered by FAST.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,23(7),075008.
MLA Guo, Ziping,et al."Single-pulse Emission Variation of Two Pulsars Discovered by FAST".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 23.7(2023):075008.
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