Rotating visco-polytropic models: Dissipative effects under the influence of a toroidal magnetic field
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Publication:1905407
DOI10.1007/BF00627551zbMath0836.76095MaRDI QIDQ1905407
V. S. Geroyannis, M. G. Sidiras
Publication date: 8 May 1996
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Gas dynamics (general theory) (76N15) General theory of rotating fluids (76U05) Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)
Cites Work
- An iterative technique for computing rotating visco-polytropic models
- A second-order perturbation theory for differentially rotating gaseous polytropes
- Equilibrium of self-gravitating polytropic cylinders with a magnetic field
- Structure-distortion of polytropic stars by differential rotation: Third- order perturbation theory
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