Institutional Repository of Radio Astronomy Research Laboratory
| Polarization and single-pulse micro-structure studies of Rotating Radio Transient J0139+3336 with FAST | |
Dang, S. J.1,2,3; Yuan, J. P.4 ; Shang, L. H.1,3; Xu, X.1,3; Tedila, H. M.4,5; Wen, Z. G.4,6,7; Yan, W. M.4; Bai, J. T.4,5; Li, Q. Y.1,3; Xiao, S.1,3; Zhao, R. S.1,3; Zhi, Q. J.1,3; Dong, A. J.1,3; Wu, Q. D.4,5; Rukiye, Rejep8; Zhang, D. D.1,3; Yang, H.1,3; Wu, C. B.1; Yuen, R.4
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| 2024-01-23 | |
| Source Publication | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| ISSN | 0035-8711 |
| Volume | 528Issue:2Pages:1213-1222 |
| Contribution Rank | 4 |
| Abstract | The study of polarization and micro-structure is very important for understanding the radiation mechanism of Rotating Radio Transients (RRATs). Due to the limitations of telescope sensitivity and time resolution, studies of the polarization and micro-structure of RRATs have been rare in the past. In this work, we report on a high-time resolution and full polarization observation of RRAT J0139+3336 with the Five-hundred-meter Aperture Spherical Radio Telescope (FAST). A total of 96 burst pulses were detected in the 3-h observation. The degrees of linear and circular polarization and the shape of the polarization position angle (PPA) of the single pulses vary significantly. The average profile displays a small degree of linear and circular polarization, and the PPA exhibits a remarkably smooth and steep S-shaped curve, which are also characteristics of pulsars. The circular polarization in some single pulses demonstrates a clear sign change. We discuss the geometric structure of the emission beam based on the results from fitting the RVM model to the changes in the PPA. Using an autocorrelation analysis, the quasi-periodic micro-structure in the single pulse emission is detected with a median period of about 0.91 ms. We show that the position of RRAT J0139+3336 on the P-P mu diagram falls in the normal pulsar (NP) region . The radio emission of RRAT J0139+3336 shows unique properties, such as the sign change in the circular polarization and quasi-periodicity in the micro-structure, which will provide important clues to the emission mechanism of RRATs. |
| Keyword | pulsars: individual: RRAT J0139+3336 |
| DOI | 10.1093/mnras/stae046 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | QUASI-PERIODIC MICROSTRUCTURE ; EMISSION ; GEOMETRY ; POLARIMETRY ; DISCOVERY ; MODEL |
| Funding Project | Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-4] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-2] ; Guizhou Province Science and Technology Foundation[ZK[2022]304] ; Scientific Research Project of the Guizhou Provincial Education[KY[2022]132] ; Scientific Research Project of the Guizhou Provincial Education[KY[2022]137] ; Scientific Research Project of the Guizhou Provincial Education[KY[2022]123] ; National SKA Program of China[2022SKA0130100] ; National SKA Program of China[2020SKA0120100] ; National SKA Program of China[2020SKA0120200] ; Academic New Seedling Fund Project of Guizhou Normal University[[2022]B18] ; National Natural Science Foundation of China[11873080] ; National Natural Science Foundation of China[U1731238] ; National Natural Science Foundation of China[11565010] ; National Natural Science Foundation of China[12103013] ; National Natural Science Foundation of China[U1838109] ; National Natural Science Foundation of China[U1831120] ; National Natural Science Foundation of China[12273008] ; National Natural Science Foundation of China[12041303] ; National Natural Science Foundation of China[12041304] ; National Natural Science Foundation of China[12288102] ; Foundation of Guizhou Provincial Education Department[KY(2020)003] ; Foundation of Guizhou Provincial Education Department[KY(2021)303] ; Guizhou Province Science and Technology Support Program[[2023] General 333] ; 2021 project Xinjiang Uygur Autonomous Region of China for Tianshan elites ; Key Laboratory of Xinjiang Uygur Autonomous Region[2020D04049] ; CAS Jianzhihua project ; National Key Program for Science and Technology Research and Development[2022YFC2205201] ; open program of the Key Laboratory of Xinjiang Uygur Autonomous Region[2020D04049] ; Operation, Maintenance, and Upgrading Fund for Astronomical Telescopes and Facility Instruments Ministry of Finance of China (MOF) |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001149830800011 |
| Publisher | OXFORD UNIV PRESS |
| Funding Organization | Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Guizhou Province Science and Technology Foundation ; Scientific Research Project of the Guizhou Provincial Education ; National SKA Program of China ; Academic New Seedling Fund Project of Guizhou Normal University ; National Natural Science Foundation of China ; Foundation of Guizhou Provincial Education Department ; Guizhou Province Science and Technology Support Program ; 2021 project Xinjiang Uygur Autonomous Region of China for Tianshan elites ; Key Laboratory of Xinjiang Uygur Autonomous Region ; CAS Jianzhihua project ; National Key Program for Science and Technology Research and Development ; open program of the Key Laboratory of Xinjiang Uygur Autonomous Region ; Operation, Maintenance, and Upgrading Fund for Astronomical Telescopes and Facility Instruments Ministry of Finance of China (MOF) |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/5779 |
| 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 Author | Dang, S. J.; Shang, L. H.; Zhi, Q. J. |
| Affiliation | 1.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550001, Peoples R China 2.Guizhou Univ, Guizhou Radio Astron Observ, Guiyang 550025, Peoples R China 3.Guizhou Prov Key Lab Radio Astron & Data Proc, Guiyang 550001, Peoples R China 4.Chinese Acad Sci, XinJiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 5.Univ Chinese Acad Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China 6.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China 7.Key Lab Microwave Technol, Urumqi 830011, Xinjiang, Peoples R China 8.Chinese Acad Sci, CAS Key Lab FAST, NAOC, Beijing 100101, Peoples R China |
| Recommended Citation GB/T 7714 | Dang, S. J.,Yuan, J. P.,Shang, L. H.,et al. Polarization and single-pulse micro-structure studies of Rotating Radio Transient J0139+3336 with FAST[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2024,528(2):1213-1222. |
| APA | Dang, S. J..,Yuan, J. P..,Shang, L. H..,Xu, X..,Tedila, H. M..,...&Yuen, R..(2024).Polarization and single-pulse micro-structure studies of Rotating Radio Transient J0139+3336 with FAST.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,528(2),1213-1222. |
| MLA | Dang, S. J.,et al."Polarization and single-pulse micro-structure studies of Rotating Radio Transient J0139+3336 with FAST".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 528.2(2024):1213-1222. |
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| Dang-2024-Polarizati（1450KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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