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The Dynamics of Globular Clusters in High Eccentricity Orbits

Published online by Cambridge University Press:  19 July 2016

R. K. Bhatia
R. K. Bhatia*
Affiliation:
Royal Observatory, Edinburgh

Extract

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The aim of the present work is two-fold: 1) To study the effect of the tidal field of the Galactic bulge on a cluster in a high eccentricity plunging orbit with half-mass density nearly equal to the Roche density; 2) To estimate the tidal or limiting radius for such orbits.

Type
Chapter IX. Poster Papers on Cluster Systems in Distant Galaxies. Deep Photometry and CM Diagrams
Information
Symposium - International Astronomical Union , Volume 126: The Harlow-Shapley Symposium on Globular Cluster Systems in Galaxies , 1988 , pp. 637 - 638
Copyright
Copyright © Kluwer 1988 

References

REFERENCES

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