The structure of motion in a 4-component galaxy mass

DOI10.1007/BF00637396zbMath0902.70008MaRDI QIDQ1371348

N. D. Caranicolas

Publication date: 16 December 1998

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

nucleusbulgechaotic orbitsaxially symmetric galaxy modellow angular momentum stars

Mathematics Subject Classification ID

Strange attractors, chaotic dynamics of systems with hyperbolic behavior (37D45) Galactic and stellar structure (85A15) Celestial mechanics (70F15)

Related Items (4)

Periodic motion in non-axially symmetric galaxies ⋮ Chaos in elliptical galaxy models ⋮ Painlevé's analysis, integrability and detecting chaos-order-chaos transition by the SALI and mLE methods of three-dimensional Armbruster Guckenheimer Kim galactic potential ⋮ Determining the nature of orbits in disk galaxies with non-spherical nuclei

Cites Work

• The Lissajous transformation. I: Basics
• A mapping for the study of the 1/1 resonance in a galactic type Hamiltonian

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