On the three-dimensional shapes of elliptical galaxies

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Celestial Mechanics, Elliptical Galaxies, Galactic Rotation, Stellar Structure, Angular Velocity, Equilibrium, Flattening, Kinetic Energy, Moment Distribution, Velocity Distribution

Scientific paper

The paper considers the hypothesis that elliptical galaxies are oblate axisymmetric objects flattened by rotation. It was found that (1) rotation does not flatten axisymmetric elliptical galaxies appreciably and elliptical galaxy models can rotate rapidly and yet show little flattening, (2) several systems remained axisymmetric when the quantity t used as a measure of rotation was greater than 0.14, and (3) models with similar shapes can have quite different internal dynamics.

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