Tree-ring structure of Galactic bar resonance in N-body simulations
Rimpei Chiba, Michiko Fujii, Junichi Baba, John Dubinski, and Ralph Sch\"onrich

TL;DR
This study uses N-body simulations to show that the galactic bar's resonant 'tree-ring' phase-space structure persists despite various perturbations, indicating a bar's spin-down and dark matter halo influence.
Contribution
It demonstrates the robustness of the tree-ring resonance structure in realistic galactic environments, even with spiral arms and satellite interactions.
Findings
Tree-ring structure remains visible despite perturbations.
Resonance captures stars sequentially from inner to outer disk.
Presence of the structure implies a dark matter halo facilitating bar spin-down.
Abstract
We study the structure and evolution of the galactic bar's resonant phase-space in self-consistent N-body simulations of the Milky Way, with and without perturbations from the Sagittarius dwarf galaxy. In an idealized disk evolution model in which stars are perturbed solely by a bar that spins down due to dynamical friction against the dark matter halo, it is predicted that stars trapped in the bar's corotation resonance form a characteristic `tree-ring' structure in phase space: as the resonance expands in volume while sweeping outwards, it sequentially captures surrounding stars at its surface, such that stars captured earlier in the inner disk are found preferentially near the core of the resonance. However, it has not been clear whether such a structure persists in a more realistic galactic disk subject to a variety of time-dependent perturbations, in particular those by spiral arms…
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