The Emission Properties of RRAT J0139+3336 at 1.25 GHz
文献类型:期刊论文
作者 | Xie, Jintao4,5; Wang, Jingbo1,2,3![]() ![]() ![]() ![]() |
刊名 | ASTROPHYSICAL JOURNAL LETTERS
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出版日期 | 2022-11-01 |
卷号 | 940期号:1页码:8 |
ISSN号 | 2041-8205 |
DOI | 10.3847/2041-8213/ac9f37 |
通讯作者 | Wang, Jingbo(1983wangjingbo@163.com) |
英文摘要 | Rotating Radio Transients are a relatively new subclass of pulsar characterized by sporadic bursting emission of single pulses. Here, we present a single-pulse analysis of a rotating radio transient, RRAT J0139+3336, using Five-hundred-meter Aperture Spherical radio Telescope at 1250 MHz. Within 3.32 hr of continuous observation, 152 single pulses were detected in RRAT J0139+3336, with the pulse rate of 45 pulses per hour. We perform a spectral analysis on the single pulses of this pulsar for the first time, finding its mean spectral indices to be -3.2 +/- 0.2, which is steeper than most known pulsars. On a single-pulse basis, we produce the first polarimetric profile of this pulsar, which fits well with the rotating vector model. The single pulses are clearly affected by diffractive scintillation with a characteristic scintillation bandwidth of v (sc) = 28 +/- 9 MHz. The pulse energy distribution for RRAT J0139+3336 can be described by a log-normal model. |
WOS关键词 | SINGLE-PULSE ; RADIO ; POLARIZATION ; UNIVERSE ; LOFAR ; MODEL |
资助项目 | National Natural Science Foundation of China[12041304] ; National SKA Program of China[2020SKA0120100] ; 201* Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents ; CAS Jianzhihua project ; Operation, Maintenance, and Upgrading Fund for Astronomical Telescopes and Facility Instruments ; Ministry of Finance of China (MOF) |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000888574400001 |
出版者 | IOP Publishing Ltd |
资助机构 | National Natural Science Foundation of China ; National SKA Program of China ; 201* Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents ; CAS Jianzhihua project ; Operation, Maintenance, and Upgrading Fund for Astronomical Telescopes and Facility Instruments ; Ministry of Finance of China (MOF) |
源URL | [http://ir.xao.ac.cn/handle/45760611-7/4954] ![]() |
专题 | 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 |
通讯作者 | Wang, Jingbo |
作者单位 | 1.Xinjiang Key Lab Radio Astrophys, Urumqi 830011, Xinjiang, Peoples R China 2.Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Xinjiang, Peoples R China 3.Lishui Univ, Inst Optoelect Technol, Lishui 323000, Zhejiang, Peoples R China 4.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 5.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China |
推荐引用方式 GB/T 7714 | Xie, Jintao,Wang, Jingbo,Wang, Na,et al. The Emission Properties of RRAT J0139+3336 at 1.25 GHz[J]. ASTROPHYSICAL JOURNAL LETTERS,2022,940(1):8. |
APA | Xie, Jintao,Wang, Jingbo,Wang, Na,Kou, Feifei,Wang, Shuangqiang,&Sun, Shengnan.(2022).The Emission Properties of RRAT J0139+3336 at 1.25 GHz.ASTROPHYSICAL JOURNAL LETTERS,940(1),8. |
MLA | Xie, Jintao,et al."The Emission Properties of RRAT J0139+3336 at 1.25 GHz".ASTROPHYSICAL JOURNAL LETTERS 940.1(2022):8. |
入库方式: OAI收割
来源:新疆天文台
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