Structure and dynamics of two-dimensional oval configurations

Details Structure and dynamics of two-dimensional oval configurations Structure and dynamics of two-dimensional oval configurations

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.170..381t&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astrophysics

1

Angular Momentum, Computerized Simulation, Disk Galaxies, Elliptical Galaxies, Gravitational Collapse, Gravitational Fields, Computer Programs, Ellipticity, Galactic Structure, Space Plasmas, Star Clusters

Scientific paper

Preliminary results are presented of 100,000-body simulations of gravitational plasmas. Results are illustrated by diagrams showing for an individual computer experiment, the excitation of an oscillatory mode of the oval equilibrium configuration. Results are further illustrated by a diagram showing ellipticity as a function of angular momentum for a sequence of configurations of given particle number, illustrating the transition from rotationally symmetric to oval equilibrium configurations.

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