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Fluid Techniques and Evolution of Anisotropy

Published online by Cambridge University Press:  25 May 2016

Rainer Spurzem
Rainer Spurzem*
Affiliation:
Institut für Astronomie und Astrophysik der Universität, Olshausenstraße 40, D-24098 Kiel e-mail: supas028@astrophysik.uni-kiel.d400.de

Abstract

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Fluid dynamical techniques to model the dynamical evolution of star clusters, and their successors, gaseous models using an equation of heat conductivity to model relaxation effects, including anisotropy, are presented. The historical merits of such models are reviewed as well as the current status of their credibility, based on quantitative comparisons with other methods, like orbit-averaged Fokker-Planck solutions and direct N-body simulations.

Information

Type
Stellar Dynamics, Models
Information
Symposium - International Astronomical Union , Volume 174: Dynamical Evolution of Stars Clusters , 1996, pp. 111 - 120
Copyright
Copyright © Kluwer 1996 

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