Models of white dwarfs under rapid uniform or differential rotation; Numerical approach - The approximative phase

Details Models of white dwarfs under rapid uniform or differential rotation; Numerical approach - The approximative phase Models of white dwarfs under rapid uniform or differential rotation; Numerical approach - The approximative phase

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.149..313g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 149, no. 2, Nov. 1988, p. 313-322.

Statistics

Computation

8

Computational Astrophysics, Stellar Models, Stellar Rotation, White Dwarf Stars, Differential Equations, Perturbation Theory

Scientific paper

Chandrasekhar's (1939) perturbation theory on rotating white dwarfs has been extended and generalized in order to investigate rapid and critical rotations. The present work focuses on the approximate phase of the method, and it includes terms up to third order in the perturbation parameter. A generalized model of rotation is proposed which includes as subcases both uniform and differential rotation.

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