NASA NTRS · 19830061834
The Riemann disks. II - Stability
Abstract
The Riemann disks are the two-dimensional analogs of the Riemann S-type ellipsoids. They form a simple yet rich family of galactic bar models. A method is developed to find their normal modes to arbitrary order, and the stability analysis is carried out for all modes with order not greater than 5.
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Weinberg, M. D.. 1983-08-15. The Riemann disks. II - Stability. https://ntrs.nasa.gov/citations/19830061834
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