Orbital tori for non-axisymmetric galaxies
Our Galaxy's bar makes the Galaxy's potential distinctly non-axisymmetric. All orbits are affected by non-axisymmetry, and significant numbers are qualitatively changed by being trapped at a resonance with the bar. Orbital tori are used to compute these effects. Thick-disc orbits are no le...
| मुख्य लेखक: | |
|---|---|
| स्वरूप: | Journal article |
| प्रकाशित: |
Oxford University Press
2017
|