Abstract
We deal with orbits of stars in galaxies (1) on the plane of symmetry of a spiral galaxy (2) on the meridian plane of an axisymmetric galaxy and (3) three-dimensional orbits in non-axisymmetric galaxies. The theory of the “third integral” explains the ordered motions- However, there are also stochastic motions that play an important role near resonances. The transition to stochasticity is studied. Finally some new types of phenomena that appear in 3-dimensional systems are discussed.
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Contopoulos, G. (1985). Nonlinear Problems in Stellar Dynamics. In: Claro, F. (eds) Nonlinear Phenomena in Physics. Springer Proceedings in Physics, vol 3. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-93289-2_9
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DOI: https://doi.org/10.1007/978-3-642-93289-2_9
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