Vertical Phase Mixing across the Galactic Disk
Zhao-Yu Li (SJTU)

TL;DR
This study uses combined LAMOST and Gaia data to analyze vertical phase mixing in the Galactic disk, revealing that guiding radius better traces phase space snail shells than current radius, with implications for understanding Galactic dynamics.
Contribution
It demonstrates that guiding radius is a more effective parameter than current radius for tracing phase space snail shells, supported by observational data and simulations.
Findings
Guiding radius enhances snail shell clarity and wraps.
Snail shell features are sharper when using guiding radius.
External perturbation timing estimated at 500-700 Myr ago.
Abstract
By combining the {\it LAMOST} and {\it Gaia} data, we investigate the vertical phase mixing across the Galactic disk. Our results confirm the existence of the phase space snail shells (or phase spirals) from 6 to 12 kpc. We find that grouping stars by the guiding radius (), instead of the present radius () further enhances the snail shell signal in the following aspects: (1) clarity of the snail shell shape is increased; (2) more wraps of the snail shell can be seen; (3) the phase spaces are less affected by the lack of stars closer to the disk mid-plane due to extinction; (4) the phase space snail shell is amplified in greater radial ranges. Compared to the -based snail shell, the quantitatively measured shapes are similar, except that the -based snail shells show more wraps with better contrast. These lines of evidence lead to the conclusion that the guiding radius…
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