# Classifying orbits in galaxy models with a prolate or an oblate dark matter halo component

@article{Zotos2014ClassifyingOI, title={Classifying orbits in galaxy models with a prolate or an oblate dark matter halo component}, author={Euaggelos E. Zotos}, journal={Astronomy and Astrophysics}, year={2014}, volume={563} }

We explore the nature of orbits of stars moving in the meridional plane $(R,z)$ of an axially symmetric galactic model with a disk, a spherical nucleus, and a flat biaxial dark matter halo component. In particular, we study the influence of all the involved parameters of the dynamical system, by computing both the percentage of chaotic orbits and the percentages of orbits of the main regular resonant families in each case. To distinguish between ordered and chaotic motion, we use the smaller…

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