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Rapidly rotating stars in shellular rotation

Auteur

Roxburgh Ian

Institution

Queen Mary University of London

Theme

Solar and stellar modelling
Auteur(s) supplémentaire(s)None
Institution(s) supplémentaire(s)N/A

Abstract

We present a method of constructing 2 dimensional models of rapidly rotating stars where the angular velocity is constant on isobars or isotherms
We present results for particular models.
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