Disks Controlling Chaos in a 3D Dynamical Model for Elliptical Galaxies
A 3D dynamical model with a quasi-homogeneous core and a disk component is used for the chaos control in the central parts of elliptical galaxy. Numerical experiments in the 2D system show a very complicated phase plane with a large chaotic sea, considerable sticky layers and a large number of islan...
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| Format: | Article |
| Language: | English |
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De Gruyter
2011-03-01
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| Series: | Open Astronomy |
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| Online Access: | https://doi.org/10.1515/astro-2017-0270 |