Orbital tori for non-axisymmetric galaxies

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...

書目詳細資料
主要作者:	Binney, J
格式:	Journal article
出版:	Oxford University Press 2017

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