Rotational Evolution of PSR J2251-3711 (The Second Slowest Radio Pulsar)

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	Rotational Evolution of PSR J2251-3711 (The Second Slowest Radio Pulsar)
	Kou,F. F.2,3; Tong,H.1
刊名	Research Notes of the AAS
	2019-11-01
卷号	3 期号:11
关键词	Radio pulsars Pulsars Magnetars Stellar magnetic fields
DOI	10.3847/2515-5172/ab595f
语种	英语
出版者	The American Astronomical Society
WOS记录号	IOP:2515-5172-3-11-AB595F
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/28649]
专题	中国科学院国家天文台
作者单位	1.School of Physics and Electronic Engineering, Guangzhou University, Guangzhou 510006, People’s Republic of China; htong_2005@163.com 2.Xinjiang Astronomical Observatories, Chinese Academy of Sciences, Urumqi 830011, People’s Republic of China 3.CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People’s Republic of China
推荐引用方式 GB/T 7714	Kou,F. F.,Tong,H.. Rotational Evolution of PSR J2251-3711 (The Second Slowest Radio Pulsar)[J]. Research Notes of the AAS,2019,3(11).
APA	Kou,F. F.,&Tong,H..(2019).Rotational Evolution of PSR J2251-3711 (The Second Slowest Radio Pulsar).Research Notes of the AAS,3(11).
MLA	Kou,F. F.,et al."Rotational Evolution of PSR J2251-3711 (The Second Slowest Radio Pulsar)".Research Notes of the AAS 3.11(2019).