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Anisotropy in ω Centauri and 47 Tucanae

Published online by Cambridge University Press:  19 July 2016

G. Meylan
G. Meylan*
Affiliation:
University of California, Berkeley

Abstract

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The southern sky gives us the great opportunity to observe two among the brightest and nearest globular clusters of the Galaxy: ω Cen and 47 Tuc. For these giant clusters, we present the comparison between observations and King-Michie multi-mass dynamical models with anisotropy in the velocity dispersion. A more comprehensive description of this work is to be published (Meylan 1986a,b).

Type
Chapter X. Poster Papers on Formation and Evolution of Globular Clusters
Information
Symposium - International Astronomical Union , Volume 126: The Harlow-Shapley Symposium on Globular Cluster Systems in Galaxies , 1988 , pp. 663 - 664
Copyright
Copyright © Kluwer 1988 

References

REFERENCES

Mayor, M., Imbert, M., Anderson, J., Ardeberg, A., Baranne, A., Benz, W., Ishci, E., Lindgren, H., Martin, N., Maurice, E., Meylan, G., Nordström, B. and Prévot, L. 1983, 1986 Astron. Astrophys. Suppl. 54, 495 and in press.Google Scholar
Meylan, G. 1968a,b, in preparation.Google Scholar