Chandrasekhar's perturbation method-oriented theories Third-order results for uniformly and differentially rotating polytropic stars; reliability and accuracy of first- and second-order results for uniform rotation

Details Chandrasekhar's perturbation method-oriented theories Third-order results for uniformly and differentially rotating polytropic stars; reliability and accuracy of first- and second-order results for uniform rotation Chandrasekhar's perturbation method-oriented theories Third-order results for uniformly and differentially rotating polytropic stars; reliability and accuracy of first- and second-order results for uniform rotation

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...299..695g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 299, Dec. 15, 1985, p. 695-705.

Statistics

Computation

16

Computational Astrophysics, Perturbation Theory, Polytropic Processes, Stellar Rotation, Stellar Structure, Computer Programs, Fortran, Numerical Integration, Stellar Rotation

Scientific paper

The aim of this investigation is the computation, by implementation of algorithms of a third-order perturbation theory developed in an earlier paper, of numerical results that represent quantitatively the distortion of the structure of a polytropic star, distortion owing to either uniform or differential rapid rotation. The results presented are systematically compared with those of previous investigations. Reliability and accuracy of firstand second-order results are also discussed. The FORTAN program implementing the codes of the theory is extensively described and specifically documented.

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