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Gravothermal catastrophe in rotating galaxies
Authors:M Clutton-Brock
Institution:(1) Astronomy Centre, University of Sussex, England;(2) Present address: University of Newcastle-upon-Tyne, England
Abstract:Violent relaxation in a rotating galaxy can lead to a core-halo, system. In order to understand this, a very, crude model is studied in which all details are ignored, and only the dimensions of physical quantities are retained. The behaviour depends on the ratio eegr of the potential in the core to the potential in the halo. When eegr>5/2, the core contracts; when eegr>5, the contraction is a runaway process, or lsquogravothermal catastrophersquo.
Keywords:
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