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Gaseous Models

Published online by Cambridge University Press:  04 August 2017

Daiichiro Sugimoto
Daiichiro Sugimoto*
Affiliation:
Department of Earth Science and Astronomy, College of Arts and Sciences, University of Tokyo

Abstract

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We can understand physics of self-gravitating system in terms of gaseous models in so far that their global natures and effects of self-gravity are concerned. Here summarized what are known in idealized gaseous models. They include gravothermal collapse/expansion in linear and non-linear regimes, and post-collapse evolution with gravothermal oscillation. Also discussed are their relations with discrete system and with treatment in statistical mechanics.

Type
May 30: Model System in the Point-Mass Approximation
Information
Symposium - International Astronomical Union , Volume 113: Dynamic of Stars Clusters , 1985 , pp. 207 - 218
Copyright
Copyright © Reidel 1985 

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