The Riemann disks. II - Stability

Details The Riemann disks. II - Stability The Riemann disks. II - Stability

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...271..595w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 271, Aug. 15, 1983, p. 595-603.

Astronomy and Astrophysics

Astrophysics

10

Astronomical Models, Disk Galaxies, Dynamic Stability, Galactic Structure, Ellipsoids, Hydrodynamics, Modal Response, Perturbation Theory, Poisson Equation

Scientific paper

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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