Ellipticity of slowly rotating configurations

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Models, Roche Limit, Rotating Fluids, Potential Theory

Scientific paper

The upper and lower bounds for m/s, where m is ratio of centrifugal
force to the gravitational force at the equator, and s is the
ellipticity of the uniformly rotating fluid is presented. To this end,
the integral equation by Clairaut is used.

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