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Structure-distortion of polytropic stars by differential rotation: Third-order perturbation theory
Authors:V. S. Geroyannis  G. A. Antonakopoulos
Affiliation:(1) Department of Astronomy, University of Patras, Greece;(2) Present address: Department of Mechanics, University of Patras, Greece
Abstract:In order to specify the structure of a rapidly and differentially rotating gaseous polytrope, we extend Chandrasekhar's perturbation theory to include third-order terms in the perturbation parameter. In the present paper, the theory developed is required for a subsequent numerical treatment of the structure-determination.This research was supported by the Research Development Project of the University of Patras, Greece.
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