An iterative technique for computing rotating white dwarf models

Details An iterative technique for computing rotating white dwarf models An iterative technique for computing rotating white dwarf models

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apjs...90..501g&link_type=abstract

Astrophysical Journal Supplement Series, vol. 90, no. 1, p. 501-510

Statistics

Computation

9

Computation, Computational Astrophysics, Iterative Solution, Stellar Models, Stellar Rotation, White Dwarf Stars, Differential Equations, Numerical Analysis, Numerical Integration, Rigid Rotors, Spherical Coordinates

Scientific paper

This paper has a twofold purpose. First, it aims at extending and applying the so-called complex-plane iterative technique (CIT) to the computation of classical white dwarf models distorted by rotation (either rigid or differential), and thus at calculating various significant physical characteristics of such models. Second, it aims at comparing the results of CIT with corresponding results of other elaborate methods and thus at establishing the reliability of this technique.

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