The equilibrium structure of loaded rotating polytropes

Details The equilibrium structure of loaded rotating polytropes The equilibrium structure of loaded rotating polytropes

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983acaps...3...55f&link_type=abstract

(Acta Astrophysica Sinica, vol. 3, no. 1, 1983, p. 55-65) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 7, June 1983

Astronomy and Astrophysics

Astrophysics

Celestial Bodies, Equilibrium Equations, Polytropic Processes, Rotating Fluids, Angular Velocity, Galactic Structure, Perturbation Theory, Stellar Structure

Scientific paper

The equilibrium structure of rotating polytropes with a compact core has been studied by means of Chandrasekhar's first-order perturbation theory. Several numerical solutions are given. The results show that the larger the core mass, the smaller the critical central angular velocity will be, and for the same angular velocity, the larger the core mass, the more oblate the rotation ellipsoid will be.

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