# Dissecting the Phase Space Snail Shell

**Authors:** Zhao-Yu Li, Juntai Shen (Shanghai Jiao Tong Univ. & Shanghai, Astronomical Obs.)

arXiv: 1904.03314 · 2020-02-26

## TL;DR

This study investigates the snail shell pattern in the Gaia DR2 data's phase space, revealing its dependence on orbit temperature and supporting a satellite-disk encounter origin over internal perturbations.

## Contribution

It provides new insights into the origin and properties of phase space snail shells, emphasizing the role of orbit temperature and external perturbations.

## Key findings

- Snail shell exists mainly in colder orbits with low radial action.
- The snail shell weakens and disappears in hotter, dynamically 'hotter' orbits.
- The results support a satellite-disk encounter scenario over internal bar buckling as the origin.

## Abstract

The on-going vertical phase mixing, manifesting itself as a snail shell in the $Z-V_{Z}$ phase space, has been discovered with the Gaia DR2 data. To better understand the origin and properties of the phase mixing process, we study the vertical phase-mixing signatures in arches (including the classical ``moving groups'') of the $V_{R}-V_{\phi}$ phase space near the Solar circle. Interestingly, the phase space snail shell exists only in the arches with $|V_{\phi} - V_{\rm LSR}| \lesssim 30$ km/s, i.e., stars on dynamically ``colder'' orbits. The snail shell becomes much weaker and eventually disappears for increasingly larger radial action ($J_{R}$), quantifying the ``hotness'' of orbits. Thus one should pay closer attention to the colder orbits in future phase mixing studies. We also confirm that the Hercules stream has two branches (at fast and slow $V_{\phi}$), which may not be explained by a single mechanism, since only the fast branch shows the prominent snail shell feature. The hotter orbits may have phase-wrapped away already due to the much larger dynamical range in radial variation to facilitate faster phase mixing. To explain the lack of a well-defined snail shell in the hotter orbits, the disk should have been perturbed at least $500$ Myr ago. Our results offer more support to the recent satellite-disk encounter scenario than the internal bar buckling perturbation scenario as the origin of the phase space mixing. Origin of the more prominent snail shell in the $V_{\phi}$ color-coded phase space is also discussed.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1904.03314/full.md

## Figures

17 figures with captions in the complete paper: https://tomesphere.com/paper/1904.03314/full.md

## References

70 references — full list in the complete paper: https://tomesphere.com/paper/1904.03314/full.md

---
Source: https://tomesphere.com/paper/1904.03314