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The evolution of the magnetic inclination angle as an explanation of the long term red timing-noise of pulsars
Yi SX(易疏序); Zhang SN(张双南); Yi; S.-X. and S.-N. Zhang
2015
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
EISSN1365-2966
Volume454Issue:4Pages:3674-3678
Corresponding Author张双南
SubtypeArticle
KeywordPulsars: General
DOI10.1093/mnras/stv2261
Indexed BySCI ; INSPIREHEP ; ADS
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000368001600027
ADS Bibcode2015MNRAS.454.3674Y
ADS URLhttps://ui.adsabs.harvard.edu/abs/2015MNRAS.454.3674Y
ADS CITATIONShttps://ui.adsabs.harvard.edu/abs/2015MNRAS.454.3674Y/citations
inspireid1395063
inspireURLhttps://inspirehep.net/literature/1395063
Citation statistics
Cited Times:10 [INSPIRE]
Cited Times:11 [ADS]
Document Type期刊论文
Identifierhttp://ir.ihep.ac.cn/handle/311005/229035
Collection粒子天体物理中心
Recommended Citation
GB/T 7714
Yi SX,Zhang SN,Yi,et al. The evolution of the magnetic inclination angle as an explanation of the long term red timing-noise of pulsars[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2015,454(4):3674-3678.
APA 易疏序,张双南,Yi,&S.-X. and S.-N. Zhang.(2015).The evolution of the magnetic inclination angle as an explanation of the long term red timing-noise of pulsars.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,454(4),3674-3678.
MLA 易疏序,et al."The evolution of the magnetic inclination angle as an explanation of the long term red timing-noise of pulsars".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 454.4(2015):3674-3678.
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