A model for tidally driven eccentric instabilities in fluid disks

• 1 November 1991
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 381, 259-267
• https://doi.org/10.1086/170647

Abstract

Keywords

• ASTRONOMICAL MODELS
• FLUID DYNAMICS
• ORBITAL RESONANCES (CELESTIAL MECHANICS)
• PLANETARY RINGS
• STELLAR SYSTEMS
• ACCRETION DISKS
• DISKS (SHAPES)
• ECCENTRIC ORBITS
• HYDRODYNAMICS
• SHELL STARS
• SYSTEMS STABILITY
• TIDES
• URANUS RINGS