Instabilities of slowly rotating galaxies

Details Instabilities of slowly rotating galaxies Instabilities of slowly rotating galaxies

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nyasa.596..150m&link_type=abstract

(Galactic models; Proceedings of the 4th Florida Workshop on Nonlinear Dynamics, Gainesville, FL, Mar. 1, 2, 1989. A91-30826 12-

Astronomy and Astrophysics

Astronomy

3

Astronomical Models, Galactic Evolution, Galactic Rotation, Galactic Structure, Many Body Problem, Rotary Stability, Digital Simulation, Elliptical Galaxies, Oblate Spheroids, Prolate Spheroids, Star Clusters

Scientific paper

The location of instabilities in flattened, pressure-supported stellar
systems is discussed. Oblate, prolate, and triaxial models of slowly
rotating galaxies is examined. The role of instabilities in explaining
the structure of observed galaxies is briefly considered.

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