Third-order perturbation theory for rotating polytropic stars

Details Third-order perturbation theory for rotating polytropic stars Third-order perturbation theory for rotating polytropic stars

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...141..425g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 141, no. 2, Dec. 1984, p. 425-429.

Astronomy and Astrophysics

Astrophysics

7

Perturbation Theory, Stellar Models, Stellar Rotation, Stellar Structure, Polytropic Processes, Radii

Scientific paper

In this investigation numerical results are presented interpreting quantitatively the distortion of the structure of a polytropic body owing to rapid rotation either uniform or differential by implementation of algorithms based upon a third-order perturbation theory developed in a previous investigation. The results obtained for the case of uniform rotation are systematically compared with those of previous investigations based on various methods.

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