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Equilibria and Dynamics of Isothermal Clouds

Published online by Cambridge University Press:  04 August 2017

Chushiro Hayashi
Chushiro Hayashi*
Affiliation:
Momoyama Yogoro-cho 1, Fushimi-ku, Kyoto 612, Japan

Abstract

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First, equilibrium structure and maximum mass of a rotating isothermal cloud are described. Second, growth rate of fragmentation instability in an infinite disk and filament is presented. Finally, results of 2D and 3D simulations of collapse and fragmentation of rotating isothermal clouds are reviewed and comments are given.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 403 - 416
Copyright
Copyright © Reidel 1987 

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