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.
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This research was supported by the Research Development Project of the University of Patras, Greece.
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Geroyannis, V.S., Antonakopoulos, G.A. Structure-distortion of polytropic stars by differential rotation: Third-order perturbation theory. Astrophys Space Sci 74, 97–110 (1981). https://doi.org/10.1007/BF00642085
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DOI: https://doi.org/10.1007/BF00642085