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Rotational Evolution of PSR J2251-3711 (The Second Slowest Radio Pulsar)
Kou,F. F.1,2; Tong,H.3
2019-11-01
Source PublicationResearch Notes of the AAS
Volume3Issue:11
KeywordRadio pulsars Pulsars Magnetars Stellar magnetic fields
DOI10.3847/2515-5172/ab595f
Language英语
WOS IDIOP:2515-5172-3-11-ab595f
PublisherThe American Astronomical Society
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Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/28650
Collection中国科学院国家天文台
Affiliation1.CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People’s Republic of China
2.Xinjiang Astronomical Observatories, Chinese Academy of Sciences, Urumqi 830011, People’s Republic of China
3.School of Physics and Electronic Engineering, Guangzhou University, Guangzhou 510006, People’s Republic of China; htong_2005@163.com
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
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).
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