The 2016 glitch in the Vela pulsar

doi:10.1007/s10509-019-3499-y

CORC > 新疆天文台 > 研究单元未命名 > 射电天文研究室 > 脉冲星研究团组

	The 2016 glitch in the Vela pulsar
	Yuen, R.1,7 ; Lee, K. J.6; Yuan, J. P.1,9,10 ; Huang, Y. X.3,5; Bai, J. M.3,5; Yan, W. M.1 ; Liu, Z. Y.1 ; Chen, W.2,3,5; Xu, Y. H.2,3,4,5; Dang, S. J.1
刊名	ASTROPHYSICS AND SPACE SCIENCE
	2019
卷号	364 期号:1 页码:11
关键词	Pulsars: individual (PSR B0833-45, J0835-4510) Stars: neutron Radio: stars
ISSN号	0004-640X
DOI	10.1007/s10509-019-3499-y
产权排序	5
英文摘要	We report the detection of a glitch event in the Vela pulsar, which occurred on 12 December 2016, based on the timing data obtained from observations between January 2016 and February 2018 at frequency centered at 2256 MHz using the Kunming 40-m radio telescope. The timing solutions for the pre- and post-glitch are presented. By fitting the glitch model to the timing data, we found that the post-glitch recovery exhibits two terms with exponential decay with the time scales of 1 d and 6 d, respectively. The glitch parameters are determined with g/=1.431(2)x10-6 and g/=73.354x10-3. The value of the coupling parameter is calculated to be approximate to 0.08, implying that the core superfluid is probably not involved in this event. For the glitches with two or more terms with exponential decay in the Vela pulsar, we show that the exponential decays usually exhibit longer time scales with higher degree of glitch recovery. The post-glitch behavior in the slow-down rate is dominated by a linear decrease process. From detection of the variations in the slopes of the spin-down rates after the exponential recoveries of the 2013 and 2016 glitches, we conclude that no persistent shift was involved in the 2016 glitches.
资助项目	Commonwealth of Australia ; Strategic Priority Research Programme of Chinese Academy of Sciences[XDB23010200] ; National Natural Science Foundation of China[U1531243] ; National Natural Science Foundation of China[U1631237] ; National Natural Science Foundation of China[11573059] ; National Natural Science Foundation of China[11873080] ; National Key R&D Program of China[2017YFA0402602] ; Open Fund of Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing
WOS关键词	NEUTRON ; EVOLUTION ; DYNAMICS
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	SPRINGER
WOS记录号	WOS:000455748900002
内容类型	期刊论文
源URL	[http://ir.xao.ac.cn/handle/45760611-7/2421]
专题	脉冲星研究团组新疆天文台_射电天文研究室
通讯作者	Yuan, J. P.
作者单位	1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 3.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Yunnan, Peoples R China 4.Guizhou Prov Key Lab Radio Astron & Data Proc, Guiyang 550025, Guizhou, Peoples R China 5.Chinese Acad Sci, Yunnan Observ, Kunming 650011, Yunnan, Peoples R China 6.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 7.Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Xinjiang, Peoples R China 8.Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China 9.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China 10.Chinese Acad Sci, Ctr Astron Mega Sci, 20A Datun Rd, Beijing 100012, Peoples R China
推荐引用方式 GB/T 7714	Yuen, R.,Lee, K. J.,Yuan, J. P.,et al. The 2016 glitch in the Vela pulsar[J]. ASTROPHYSICS AND SPACE SCIENCE,2019,364(1):11.
APA	Yuen, R..,Lee, K. J..,Yuan, J. P..,Huang, Y. X..,Bai, J. M..,...&Hao, L. F..(2019).The 2016 glitch in the Vela pulsar.ASTROPHYSICS AND SPACE SCIENCE,364(1),11.
MLA	Yuen, R.,et al."The 2016 glitch in the Vela pulsar".ASTROPHYSICS AND SPACE SCIENCE 364.1(2019):11.