Statistics – Computation
Scientific paper
May 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.191..175s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 191, no. 2, May 1992, p. 175-184.
Statistics
Computation
Galactic Clusters, Gravitational Fields, Interacting Galaxies, Orbital Resonances (Celestial Mechanics), Stellar Mass, Stellar Orbits, Computational Astrophysics, Stellar Oscillations
Scientific paper
The behavior of stellar orbits is examined under the influence of a
fixed triaxial potential and a tidal force. Changes in the kinetic
energies in the principal directions are computed as a function of tidal
interaction times; the important resonances are identified. Resonant
interactions are discussed in relation to clusters of galaxies.
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