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

DOI10.1007/S10509-008-9946-9zbMath1172.85307OpenAlexW1993666467MaRDI QIDQ835524

A. K. Lal, Ankush Pathania, Cruz Mohan

Publication date: 28 August 2009

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

Full work available at URL: https://doi.org/10.1007/s10509-008-9946-9

zbMATH Keywords

Coriolis forcebinary starsrotating starsRoche equipotentialRoche limit

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Galactic and stellar dynamics (85A05)

Cites Work

• Equilibrium structures of rotationally and tidally distorted polytropic models of stars
• Effect of Coriolis force on the equilibrium structures of rotating stars and stars in binary systems
• Roche limit for homogeneous incompressible masses
• Vibrational stability of rotating stars
• Use of Roche coordinates in the problems of small oscillations of tidally distorted stellar models
• Dynamics of close binary systems
• Equilibrium structures of differentially rotating primary components of binary stars

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