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International Journal of Computer Mathematics Volume 34, 1990 - Issue 1-2
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Original Articles

An algorithm for numerical solution of the stellar hydrodynamical equations

N. W. Evans School of Mathematical Sciences, Queen Mary College, London, EI 4NS, UK
Pages 105-112 | Received 20 Dec 1989, Published online: 20 Mar 2007
 
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Abstract

The stellar hydrodynamical equations give the components of stress required to support a stellar system against gravitational collapse. The paper derives a numerical algorithm to solve the stellar hydrodynamical equations in spheroidal coordinates, widely used for galactic modelling.

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