Institutional Repository of Radio Astronomy Research Laboratory
| Timing and emission variation of PSR J1733-3716 | |
Hu, Yue1,2 ; Li, Lin1; Yuan, J. P.2,3; Dang, S. J.2,3; Wang, S. Q.2,3; Wang, Z. J.1; Yuen, R.2
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| 2020-08-24 | |
| Source Publication | ASTROPHYSICS AND SPACE SCIENCE
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| ISSN | 0004-640X |
| Volume | 365Issue:8Pages:143 |
| Contribution Rank | 2 |
| Abstract | We present analysis of the timing noise in PSR J1733-3716, which combines data from Parkes 64-m radio telescope and nearly 15 years of timing data obtained from the Nanshan 25-m radio telescope. The variations in the spin frequency and frequency derivative are determined. The fluctuation in the spin frequency is obvious with an amplitude of1.94(7)x10(-9) Hz . Variations of the integrated profile at 1369 MHz are detected with the changes occur in the relative peak intensity from the right profile component. From analysis of the single pulse data at 1382 MHz, we detect weak emission states that account for 63% of the whole data, and its duration distribution can be fitted with a power law. The pulsar also exhibits strong emission states, during which the emission shows multiple modes. This includes the normal mode, left mode and the right mode, with the time scales spanning between one and seventeen pulse periods. Such short term variability in pulses contributes to the variation of the integrated profile. Examination of the correlations between the spin parameters and the integrated profiles shows likelihood of a random distribution, which reveals that there is probably no obvious relationship between spin-down rate variations and changes of emission in this pulsar. |
| Keyword | Pulsars individual PSR J1733-3716 |
| DOI | 10.1007/s10509-020-03849-8 |
| URL | 查看原文 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | MAGNETOSPHERIC FLUCTUATIONS ; GLITCH ACTIVITY ; RADIO-EMISSION ; PULSAR ; ROTATION ; PACKAGE ; TEMPO2 ; NOISE ; MODEL |
| Funding Project | National Key R&D Program of China[2017YFA0402602] ; National Natural Science Foundation of China[11563008] ; National Natural Science Foundation of China[11873080] ; National Natural Science Foundation of China[11573059] ; Center for Astronomical Mega-Science, Chinese Academy of Sciences ; West Light Foundation of the Chinese Academy of Sciences[2016-QNXZ-B-24] ; Australian Government |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000567853400002 |
| Publisher | SPRINGER |
| Funding Organization | National Key R&D Program of China ; National Natural Science Foundation of China ; Center for Astronomical Mega-Science, Chinese Academy of Sciences ; West Light Foundation of the Chinese Academy of Sciences ; Australian Government |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/3662 |
| Collection | 射电天文研究室_脉冲星研究团组 科研仪器设备产出_利用南山26米射电望远镜（NSRT）观测数据的文章 |
| Corresponding Author | Wang, Z. J. |
| Affiliation | 1.Xinjiang Univ, Dept Phys, Urumqi 830046, Peoples R China 2.Chinese Acad Sci, Xinjiang Astron Observ, 150,Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 3.Univ Chinese Acad Sci, Beijing 100049, Peoples R China |
| First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Recommended Citation GB/T 7714 | Hu, Yue,Li, Lin,Yuan, J. P.,et al. Timing and emission variation of PSR J1733-3716[J]. ASTROPHYSICS AND SPACE SCIENCE,2020,365(8):143. |
| APA | Hu, Yue.,Li, Lin.,Yuan, J. P..,Dang, S. J..,Wang, S. Q..,...&Yuen, R..(2020).Timing and emission variation of PSR J1733-3716.ASTROPHYSICS AND SPACE SCIENCE,365(8),143. |
| MLA | Hu, Yue,et al."Timing and emission variation of PSR J1733-3716".ASTROPHYSICS AND SPACE SCIENCE 365.8(2020):143. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| Hu-2020-Timing and e（1631KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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