中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Observations of Bright Pulses from Pulsar B0031-07 at 4.82 GHz

文献类型:期刊论文

作者Wen, Z. G.6,7,8; Yuen, R.8; Wang, N.7,8; Tu, Z. Y.8; Yan, Z.5; Yuan, J. P.7,8; Yan, W. M.7,8; Chen, J. L.4,8; Wang, H. G.3,8; Shen, Z. Q.5
刊名ASTROPHYSICAL JOURNAL
出版日期2021-09-01
卷号918期号:2页码:8
ISSN号0004-637X
DOI10.3847/1538-4357/ac0e90
通讯作者Wen, Z. G.(wenzhigang@xao.ac.cn)
英文摘要We report on the detection of 146 (0.96%) bright pulses with a peak flux density >0.86 Jy from PSR B0031-07 in 4 hr of continuous observations made at 4.82 GHz, with a bandwidth of 1 GHz, using the Shanghai Tian Ma 65 m radio telescope. We find that the peak flux density distribution follows a power law with index alpha = -3.6 +/- 0.2, while the pulse energy appears to follow a logarithmic normal distribution. The bright pulses from PSR B0031-07 were observed to repeat in an irregular fashion. The intervals between bright pulses can be described with an exponentiated Weibull distribution. Furthermore, the sensitive observations at higher frequency with a short time resolution of 65.54 mu s form a reliable basis for detailed microstructure studies. Close inspection of the detected bright pulses reveals that 38 pulses exhibit well-defined quasi-periodicities. No unanimous period for the quasi-periodicities is found, and the peak flux density is independent of the micropulse width. Finally, possible physical mechanisms are discussed.
WOS关键词GIANT PULSES ; RADIO-EMISSION ; CRAB PULSAR ; MICROSTRUCTURE
资助项目Chinese National Science Foundation[U1838109] ; Chinese National Science Foundation[U1731238] ; Chinese National Science Foundation[U1831102] ; Chinese National Science Foundation[U1631106] ; Chinese National Science Foundation[11873080] ; National Natural Science Foundation of China[12041304] ; National SKA Program of China[2020SKA0120100] ; Astronomical Research Centre of the Chinese Academy of Sciences ; National Program on Key Research and Development Project[2016YFA0400804] ; Xinjiang uygur autonomous region of China ; Open Fund of Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000695450500001
出版者IOP PUBLISHING LTD
资助机构Chinese National Science Foundation ; National Natural Science Foundation of China ; National SKA Program of China ; Astronomical Research Centre of the Chinese Academy of Sciences ; National Program on Key Research and Development Project ; Xinjiang uygur autonomous region of China ; Open Fund of Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing
源URL[http://ir.xao.ac.cn/handle/45760611-7/4271]  
专题研究单元未命名
新疆天文台_射电天文研究室
射电天文研究室_数字技术实验室
通讯作者Wen, Z. G.
作者单位1.Key Lab Microwave Technol, Urumqi 830011, Xinjiang, Peoples R China
2.Xinjiang Univ, Sch Phys Sci & Technol, Urumqi 830046, Xinjiang, Peoples R China
3.Guangzhou Univ, Sch Phys & Elect Engn, Guangzhou 510006, Peoples R China
4.Yuncheng Univ, Dept Phys & Elect Engn, Yuncheng 044000, Shanxi, Peoples R China
5.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
6.Guizhou Prov Key Lab Radio Astron & Data Proc, Guiyang 550001, Guizhou, Peoples R China
7.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China
8.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
推荐引用方式
GB/T 7714
Wen, Z. G.,Yuen, R.,Wang, N.,et al. Observations of Bright Pulses from Pulsar B0031-07 at 4.82 GHz[J]. ASTROPHYSICAL JOURNAL,2021,918(2):8.
APA Wen, Z. G..,Yuen, R..,Wang, N..,Tu, Z. Y..,Yan, Z..,...&Mao, J. W..(2021).Observations of Bright Pulses from Pulsar B0031-07 at 4.82 GHz.ASTROPHYSICAL JOURNAL,918(2),8.
MLA Wen, Z. G.,et al."Observations of Bright Pulses from Pulsar B0031-07 at 4.82 GHz".ASTROPHYSICAL JOURNAL 918.2(2021):8.

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来源:新疆天文台

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