Equilibrium structures of rotationally and tidally distorted polytropic models of stars

DOI10.1007/S10509-006-9209-6zbMath1117.85318OpenAlexW2000035401MaRDI QIDQ867157

N. E. Zubov

Publication date: 15 February 2007

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-006-9209-6

zbMATH Keywords

Binary systemsEquilibrium structuresPolytropic modelsRoche equipotentialsRotating stars

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Related Items (2)

Effect of Coriolis force on the shapes of rotating stars and stars in binary systems ⋮ Effect of Coriolis force on the equilibrium structures of rotating stars and stars in binary systems

Cites Work

• Dynamics of close binary systems
• Equilibrium structures of differentially rotating primary components of binary stars
• Physical characteristics of critically distorted or almost spherically shaped rotating magnetic polytropic models

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