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Dynamical Models for Axisymmetric and Triaxial Galaxies

Published online by Cambridge University Press:  04 August 2017

Tim de Zeeuw
Tim de Zeeuw*
Affiliation:
The Institute for Advanced Study, Princeton, NJ 08540, USA

Abstract

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Non–spherical dynamical models for galaxies, and the methods for their construction, are reviewed. The theory for two–integral axisymmetric models is reasonably well developed. Stäckel models give considerable insight in the structure of both three–integral axisymmetric models and non–rotating triaxial systems. Triaxial galaxies with appreciable figure rotation require much further study. Applications to elliptical galaxies and the bulges of disk galaxies are discussed.

Type
Invited Reviews
Information
Symposium - International Astronomical Union , Volume 127: Structure and Dynamics of Elliptical Galaxies , 1987 , pp. 271 - 290
Copyright
Copyright © Reidel 1987 

References

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