Hostname: page-component-6bf8c574d5-w79xw Total loading time: 0 Render date: 2025-02-15T18:37:49.077Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Caputo, F. and Castellani, V. 1984 Monthly Notices Roy. Astron. Soc. 207, 185.CrossRefGoogle Scholar
Castellani, V. and Melchiorri, M. 1981 Astrophys. and Space Sci. 89, 289.CrossRefGoogle Scholar
Innanen, K. A., Harris, W. E. and Webbink, R. F. 1983 Astron. J. 88, 338.CrossRefGoogle Scholar