Did Sgr cause the vertical waves in the solar neighbourhood?
Morgan Bennett, Jo Bovy

TL;DR
This study develops a rapid computational method to test if the Sagittarius dwarf galaxy's passage caused vertical waves in the Milky Way's disc, concluding it likely did not based on Gaia data comparisons.
Contribution
The paper introduces a fast technique for modeling satellite-induced perturbations in galactic discs and applies it to Sgr, ruling out its role in observed vertical oscillations.
Findings
Sgr passage cannot reproduce observed vertical asymmetries.
The amplitude and wavelength of simulated perturbations do not match Gaia data.
Sgr is unlikely the cause of the phase-space spiral in the solar neighborhood.
Abstract
The vertical distribution of stars in the solar neighbourhood is not in equilibrium but contains a wave signature in both density and velocity space originating from a perturbation. With the discovery of the phase-space spiral in Gaia data release 2, determining the origin of this perturbation has become even more urgent. We develop and test a fast method for calculating the perturbation from a passing satellite on the vertical component of a part of a disc galaxy. This fast method allows us to test a large variety of possible perturbations to the vertical disc very quickly. We apply our method to the range of possible perturbations to the solar neighbourhood stemming from the recent passage of the Sagittarius dwarf galaxy (Sgr), varying its mass, mass profile, and present-day position within their observational uncertainties, and its orbit within different realistic models for the…
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