Models of white dwarfs under rapid uniform or differential rotation - Numerical results. II

Details Models of white dwarfs under rapid uniform or differential rotation - Numerical results. II Models of white dwarfs under rapid uniform or differential rotation - Numerical results. II

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apjs...75..499g&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 75, Feb. 1991, p. 499-506.

Statistics

Computation

8

Computational Astrophysics, Stellar Models, Stellar Rotation, White Dwarf Stars, Angular Velocity, Perturbation Theory, Stellar Mass

Scientific paper

A 'complex-plane strategy' and a 'multiple-partition technique' are used here to compute 'classical' white dwarf models distorted by either uniform or differential rotation. Values of some significant structure functions are given for several values of the fundamental model parameter and also for several values of the strength of differential rotation.

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