Comparison of resonant orbits. IV - The numerical results in a quasispherical galaxy (Resonance 1/1)

Details Comparison of resonant orbits. IV - The numerical results in a quasispherical galaxy (Resonance 1/1) Comparison of resonant orbits. IV - The numerical results in a quasispherical galaxy (Resonance 1/1)

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986baicz..37..358a&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 37, Nov. 1986, p. 358-363.

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Computational Astrophysics, Galaxies, Orbital Resonances (Celestial Mechanics), Resonance, Stellar Orbits, Gravitational Fields

Scientific paper

A numerical investigation is made of resonant orbits that are more or less disturbed in near-spherical galactic systems. Stellar orbits with similar resonances are studied and compared. A quasi-spherical potential with a disturbing term is assumed. In comparing three characteristics (maximum distances from the axis of symmetry, invariant curves, and surfaces of section), it is shown that three groups of orbits can be found in this case: (1) ergodic orbits, (2) 'combined' orbits, and (3) orbits with both stars remaining in the vicinity of the basic aperiodic solution.

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