Numerical function values for slowly rotating partially degenerate semirelativistic isothermal spheroids of arbitrary temperature

Astronomy and Astrophysics – Astrophysics

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Astrophysics, Stellar Rotation, Stellar Structure, White Dwarf Stars, Isothermal Processes, Oblate Spheroids, Tables (Data)

Scientific paper

Numerical function values for the structural properties of slowly rotating, partially degenerate, semirelativistic isothermal spheroids of arbitrary but constant temperature are presented. Tabulations of structural functions, of the scaled radius, mass, moment of inertia, and density, of homology functions, of the expansion, ellipticity, and oblateness, and of the rotational perturbations to the mass, density, and moment of inertia are given for several combinations of the temperature parameter (zeta), the central degeneracy parameter.

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