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Stellar models under homoaxial rotation: Eulerian equations and simulation of non-uniformly rotating stars

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Abstract

The Eulerian equations are set up for a model subject to homoaxial rotation and suitable for simulation of a non-uniformly rotating star. These equations are formulated in a non-inertial frame of reference, rotating uniformly (i.e., rigidly) with respect to the inertial common frame.

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References

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  1. Astronomy Laboratory, Department of Physics, University of Patras, Greece

    V. S. Geroyannis

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  1. V. S. Geroyannis
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Geroyannis, V.S. Stellar models under homoaxial rotation: Eulerian equations and simulation of non-uniformly rotating stars. Astrophys Space Sci 120, 43–59 (1986). https://doi.org/10.1007/BF00653899

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  • DOI: https://doi.org/10.1007/BF00653899

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