Numerical implementation of a perturbation theory up to third order for rotating polytropic stars - Structure parameters under differential rotation

Details Numerical implementation of a perturbation theory up to third order for rotating polytropic stars - Structure parameters under differential rotation Numerical implementation of a perturbation theory up to third order for rotating polytropic stars - Structure parameters under differential rotation

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...312..219g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 312, Jan. 1, 1987, p. 219-226.

Statistics

Computation

7

Computational Astrophysics, Numerical Analysis, Perturbation Theory, Polytropic Processes, Stellar Models, Stellar Rotation, Gravitational Effects, Magnetohydrodynamic Stability, Stellar Structure

Scientific paper

We present numerical results for the most significant structure
parameters of a differentially rotating polytropic star. These results
have been derived by implementation of a third-order perturbation theory
developed in a previous investigation.

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