| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1779204 | New Astronomy | 2012 | 13 Pages |
Abstract
⺠An axially symmetric galactic model with a disk-halo and a spherical nucleus is used. ⺠The galactic core hosts a dense and massive spherical nucleus. ⺠We reveal the structure of the dynamical system using a time independent model. ⺠We explore the nature of orbits in the case of the time evolving model. ⺠A theoretical analysis to support the numerically derived outcomes is also presented.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Euaggelos E. Zotos,