Revealing the dynamical behavior of stars in a prolate or oblate elliptical galaxy
We consider the motion of a test particle (star) on the meridian plane (R,z) of an elliptical galaxy with an additional central nucleus component. The shape of the elliptical galaxy can be either prolate or oblate, or even spherical by simply changing the numerical value of the flattening parameter...
| Published in: | Results in Physics |
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| Main Authors: | , , |
| Format: | Article |
| Language: | English |
| Published: |
Elsevier
2023-05-01
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| Subjects: | |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S2211379723002000 |