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| The Study of Mode-switching Behavior of PSR J0614+2229 Using the Parkes Ultra-wide-bandwidth Receiver Observations | |
Cai, Yanqing1; Dang, Shijun1,2,3 ; Yuen, Rai4; Shang, Lunhua1; Kou, Feifei4; Yuan, Jianping4; Zhang, Lei5; Zhou, Zurong6,7; Wang, Na4; Li, Qingying1; Wen, Zhigang4; Yan, Wenming4; Wang, Shuangqiang4; Sun, Shengnan4; Tedila, Habtamu Menberu5; Xiao, Shuo1,3; Xu, Xin1; Zhao, Rushuang1; Zhi, Qijun1; Dong, Aijun1; Zhang, Bing1; Li, Wei1; Ren, Yingying1; Liu, Yujia1
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| 2024-05-01 | |
| Source Publication | ASTROPHYSICAL JOURNAL
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| ISSN | 0004-637X |
| Volume | 966Issue:2Pages:241 |
| Contribution Rank | 4 |
| Abstract | In this paper we present a detailed single-pulse and polarization study of PSR J0614+2229 based on the archived data observed on 2019 August 15 (MJD 58710) and 2019 September 12 (MJD 58738) using the ultra-wide-bandwidth low-frequency receiver on the Parkes radio telescope. The single-pulse sequences show that this pulsar switches between two emission states, in which the emission of state A occurs earlier than that of state B in pulse longitude. We found that the variation in relative brightness between the two states varies temporally and both states follow a simple power law very well. Based on the phase-aligned multifrequency profiles, we found that there is a significant difference in the distributions of spectral index across the emission regions of the two states. Furthermore, we obtained the emission height evolution for the two emission states and found that, at a fixed frequency, the emission height of state A is higher than that of state B. What is even more interesting is that the emission heights of both states A and B do not change with frequency. Our results suggest that the mode switching of this pulsar is possibly caused by changes in the emission heights that alter the distributions of spectral index across the emission regions of states A and B, resulting in frequency-dependent behaviors, i.e., intensity and pulse width. |
| DOI | 10.3847/1538-4357/ad395f |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | FREQUENCY-DEPENDENCE ; RADIO ; EMISSION ; PULSARS ; MULTIFREQUENCY ; SCINTILLATION ; B0919+06 |
| Funding Project | National Natural Science Foundation of China[2022A03013-4] ; National Natural Science Foundation of China[2022A03013-2] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[ZK[2022]304] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[ZK[2023]024] ; Guizhou Province Science and Technology Foundation[[2022]132] ; Guizhou Province Science and Technology Foundation[[2022]137] ; Scientific Research Project of the Guizhou Provincial Education[12273008] ; Scientific Research Project of the Guizhou Provincial Education[U1731238] ; Scientific Research Project of the Guizhou Provincial Education[U1831120] ; Scientific Research Project of the Guizhou Provincial Education[U1838106] ; Scientific Research Project of the Guizhou Provincial Education[61875087] ; Scientific Research Project of the Guizhou Provincial Education[61803373] ; Scientific Research Project of the Guizhou Provincial Education[11303069] ; Scientific Research Project of the Guizhou Provincial Education[11373011] ; Scientific Research Project of the Guizhou Provincial Education[11873080] ; Scientific Research Project of the Guizhou Provincial Education[12103069] ; National Natural Science Foundation[2024JC-YBQN-0036] ; Natural Science Basic Research Program of Shaanxi[(2020)003] ; Foundation of Guizhou Provincial Education Department[2017 YFB 0503300] ; National Key R&D Program of China[[2016]4008] ; National Key R&D Program of China[5726-37] ; National Key R&D Program of China[[2018]5769-02] ; Foundation of Science and Technology of Guizhou Province ; Australian Government |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001218733500001 |
| Publisher | IOP Publishing Ltd |
| Funding Organization | National Natural Science Foundation of China ; 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 Natural Science Foundation ; Natural Science Basic Research Program of Shaanxi ; Foundation of Guizhou Provincial Education Department ; National Key R&D Program of China ; Foundation of Science and Technology of Guizhou Province ; Australian Government |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/6623 |
| Collection | 射电天文研究室_脉冲星研究团组 |
| Corresponding Author | Dang, Shijun; Shang, Lunhua |
| Affiliation | 1.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550025, 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 550025, Peoples R China 4.Chinese Acad Sci, XinJiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 5.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China 6.Chinese Acad Sci, Natl Time Serv Ctr, Xian 710600, Peoples R China 7.Chinese Acad Sci, Key Lab Time Reference & Applicat, Xian 710600, Peoples R China |
| Recommended Citation GB/T 7714 | Cai, Yanqing,Dang, Shijun,Yuen, Rai,et al. The Study of Mode-switching Behavior of PSR J0614+2229 Using the Parkes Ultra-wide-bandwidth Receiver Observations[J]. ASTROPHYSICAL JOURNAL,2024,966(2):241. |
| APA | Cai, Yanqing.,Dang, Shijun.,Yuen, Rai.,Shang, Lunhua.,Kou, Feifei.,...&Liu, Yujia.(2024).The Study of Mode-switching Behavior of PSR J0614+2229 Using the Parkes Ultra-wide-bandwidth Receiver Observations.ASTROPHYSICAL JOURNAL,966(2),241. |
| MLA | Cai, Yanqing,et al."The Study of Mode-switching Behavior of PSR J0614+2229 Using the Parkes Ultra-wide-bandwidth Receiver Observations".ASTROPHYSICAL JOURNAL 966.2(2024):241. |
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| Cai-2024-The Study o（2608KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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