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...
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| Formaat: | Journal article |
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Oxford University Press
2017
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