Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-12T14:23:36.889Z Has data issue: false hasContentIssue false
  • English
  • Français

Analytic Axisymmetric Dynamical Models with Three Integrals of Motion

Published online by Cambridge University Press:  04 August 2017

Herwig Dejonghe  and
Tim de Zeeuw
Herwig Dejonghe
Affiliation:
The Institute for Advanced Study, Princeton, NJ 08540
Tim de Zeeuw
Affiliation:
The Institute for Advanced Study, Princeton, NJ 08540

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.

We consider a family of inhomogeneous axisymmetric mass models with a simple gravitational potential originally introduced by Kuzmin (1956): where R2 = x2 + y2, a and c are parameters, G is the gravitational constant, and M is the total mass of the corresponding density distribution.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 127: Structure and Dynamics of Elliptical Galaxies , 1987 , pp. 497 - 498
Copyright
Copyright © Reidel 1987 

References

REFERENCES

Dejonghe, H., 1986. Physics Reports, 133, 217.Google Scholar
de Zeeuw, P.T., 1985. Mon. Not. R. astr. Soc., 216, 273.Google Scholar
de Zeeuw, P.T. & Lynden–Bell, D., 1985. Mon. Not. R. astr. Soc., 215, 713.Google Scholar
Hénon, M., 1960. Ann. d' Astrophys., 23, 474.Google Scholar
Hunter, C., 1975. Astron. J., 80, 783.CrossRefGoogle Scholar
Kalnajs, A., 1976. Astrophys. J., 205, 751.CrossRefGoogle Scholar
Kuzmin, G.G., 1956. Astr. Zh., 33, 27.Google Scholar
Kuzmin, G.G., & Kutuzov, S.A., 1962. Bull. Abastumani Astroph. Obs., 27, 82.Google Scholar
Lynden–Bell, D., 1962. Mon. Not. R. astr. Soc., 123, 447.Google Scholar