A new criterion for secular instability of rapidly rotating stars

• 1 October 1977
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 217, L49-L53
• https://doi.org/10.1086/182537

Abstract

Keywords

• SECULAR VARIATION
• ROTATION
• HYDRODYNAMICS
• MECHANICS
• MATHEMATICAL MODELS
• FLUID MECHANICS
• MOTION
• ANGULAR MOMENTUM
• INSTABILITY
• QUANTUM MECHANICS
• STARS
• GRAVITATIONAL RADIATION
• MATHEMATICAL MODEL