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Analytic Axisymmetric Dynamical Models with Three Integrals of Motion

Published online by Cambridge University Press:  04 August 2017

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

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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
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