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The globular cluster tidal radii†

Published online by Cambridge University Press:  01 October 2007

Z. Y. Wu
Z. Y. Wu*
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China email: [email protected]
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Abstract

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The orbits and theoretical tidal radii for a sample of 45 Galactic globular clusters are calculated. The orbital phase dependence between the theoretical and observed tidal radii is noted.

Keywords

Galaxy: kinematics and dynamicsglobular clusters: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S248: A Giant Step: from Milli- to Micro-arcsecond Astrometry , October 2007 , pp. 512 - 513
Copyright
Copyright © International Astronomical Union 2008

References

Hoerner, S. Von. 1957, ApJ, 125, 451CrossRefGoogle Scholar
Innanen, K. A. 1983 AJ, 88, 338CrossRefGoogle Scholar
King, I. R. 1962, AJ, 67, 471CrossRefGoogle Scholar
King, I. R. 1966, AJ, 71, 64CrossRefGoogle Scholar
Meziane, K. & Colin, J. 1996, A&A, 306, 747Google Scholar
Trager, S. C., et al. 1993, ASP-CS, 50, 347Google Scholar
Wu, Z.-Y., Shu, C.-G., & Chen, W.-P. 2003, Chin. Phys. Lett., 20, 1648Google Scholar
Wu, Z.-Y., Zhou, X., & Ma, J. 2004, Chin. Phys. Lett., 21, 418Google Scholar