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Orbital phase dependence of globular cluster's tidal radii
Wu, ZY; Zhou, X; Ma, J
2004-02-01
Source PublicationCHINESE PHYSICS LETTERS
Volume21Issue:2Pages:418-420
AbstractThe orbits for a sample of 45 galactic globular clusters are calculated using positions and spatial velocities based on recent compilations as well as new measurements of their absolute proper motions. The perigalactic positions of each cluster are used to determine their theoretical tidal radii in the given galactic model. The orbital phase dependence between the theoretical and observed tidal radii is evidenced.
Indexed BySCI
Language英语
WOS IDWOS:000189013100057
Citation statistics
Cited Times:2[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8138
Collection光学天文研究部
AffiliationChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Wu, ZY,Zhou, X,Ma, J. Orbital phase dependence of globular cluster's tidal radii[J]. CHINESE PHYSICS LETTERS,2004,21(2):418-420.
APA Wu, ZY,Zhou, X,&Ma, J.(2004).Orbital phase dependence of globular cluster's tidal radii.CHINESE PHYSICS LETTERS,21(2),418-420.
MLA Wu, ZY,et al."Orbital phase dependence of globular cluster's tidal radii".CHINESE PHYSICS LETTERS 21.2(2004):418-420.
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