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| The spin-down state change and mode change associated with glitch activity of PSR B2035+36 | |
Kou, F. F.1,2 ; Yuan, J. P.1,3; Wang, N.1,3; Yan, W. M.1; Dang, S. J.1,2
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| 2018-07-01 | |
| Source Publication | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| ISSN | 0035-8711 |
| Volume | 478Issue:1Pages:L24-L28 |
| Contribution Rank | 1 |
| Abstract | We presented timing results of PSR B2035+36 using similar to 9-yr observations with the Nanshan 25-m radio telescope. PSR B2035+ 36 was reported to exhibit significant changes in pulse profile correlated with spin-down state variations. We found that the pulsar underwent a glitch with a jump in frequency of Delta nu similar to 12.4(5) nHz around MJD 52950. Unusually, the spin-down rate increased persistently over 800 d after the glitch, and the average spin-down rate postglitch was about 9.6 per cent larger than that pre-glitch. After the glitch activity, the pulse profile became narrower and the pulsar began to switch between two emission modes, with pulse widths (W-50mean) of 8.5(7)degrees and 3.7(3)degrees, respectively. In addition to that, the relatively narrow pulse profile gradually became dominant. All of the observations indicate that there should be a connection between magnetospheric behaviour and glitch activity. We discuss one possibility of magnetosphere fluctuation triggered by the glitch event. |
| Keyword | stars: neutron pulsar: general pulsars: individual:(PSR B2035+36) |
| DOI | 10.1093/mnrasl/sly068 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | PULSAR-TIMING PACKAGE ; NEUTRON-STARS ; EVOLUTION ; TEMPO2 |
| Funding Project | National Natural Science Foundation of China[U1731238] ; National Basic Research Program of China grants 973 Programs[2015CB857100] ; National Key Research and Development Program of China[2016YFA0400800] ; National Key Research and Development Program of China[2017YFA0402602] ; Strategic Priority Research Program of the Chinese Academy of Sciences[XD23010200] ; West Light Foundation of CAS[XBBS201422] ; National Natural Science Foundation of China[U1631106] |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000450777200005 |
| Publisher | OXFORD UNIV PRESS |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/2262 |
| Collection | 射电天文研究室_脉冲星研究团组 110米口径全可动射电望远镜（QTT）_110米大口径全可动射电望远镜关键技术研究（973项目）_课题4：反射面高精度快速测量与主动面实时闭环修正 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 | Yuan, J. P. |
| Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 2.Univ Chinese Acad Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China 3.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China |
| First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Recommended Citation GB/T 7714 | Kou, F. F.,Yuan, J. P.,Wang, N.,et al. The spin-down state change and mode change associated with glitch activity of PSR B2035+36[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,478(1):L24-L28. |
| APA | Kou, F. F.,Yuan, J. P.,Wang, N.,Yan, W. M.,&Dang, S. J..(2018).The spin-down state change and mode change associated with glitch activity of PSR B2035+36.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,478(1),L24-L28. |
| MLA | Kou, F. F.,et al."The spin-down state change and mode change associated with glitch activity of PSR B2035+36".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 478.1(2018):L24-L28. |
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| Kou-2018-The spin-do（342KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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