A New Dynamical Parameter for the Study of Sticky Orbits in a 3D Galactic Model
A 3D dynamical model is used to study the motion in the central parts of an elliptical galaxy, hosting a massive and dense nucleus. Our aim is to investigate the regular or chaotic character of the motion, with emphasis in the different chaotic components, as well as the sticky regions of the dynami...
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| Format: | Article |
| Language: | English |
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De Gruyter
2011-09-01
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| Series: | Open Astronomy |
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| Online Access: | https://doi.org/10.1515/astro-2017-0301 |