Rings and Radial Waves in the Disk of the Milky Way
Yan Xu, Heidi Jo Newberg, Jeffrey L. Carlin, Chao Liu, Licai Deng,, Jing Li, Ralph Sch\"onrich, Brian Yanny

TL;DR
This paper identifies oscillating asymmetries in star counts across the Milky Way's disk, revealing concentric rings linked to disk oscillations and spiral structure, based on Sloan Digital Sky Survey data.
Contribution
It provides evidence that the Monoceros and TriAnd Rings are caused by disk oscillations and details their spatial relationships and possible connection to spiral arms.
Findings
Oscillating star count asymmetries form concentric rings around the Galactic center.
The Monoceros and TriAnd Rings are likely due to disk oscillations.
The disk exhibits non-azimuthal symmetry and possible links to spiral structure.
Abstract
We show that in the anticenter region, between Galactic longitudes of , there is an oscillating asymmetry in the main sequence star counts on either side of the Galactic plane using data from the Sloan Digital Sky Survey. This asymmetry oscillates from more stars in the north at distances of about 2 kpc from the Sun to more stars in the south at 4-6 kpc from the Sun to more stars in the north at distances of 8-10 kpc from the Sun. We also see evidence that there are more stars in the south at distances of 12-16 kpc from the Sun. The three more distant asymmetries form roughly concentric rings around the Galactic center, opening in the direction of the Milky Way's spiral arms. The northern ring, 9 kpc from the Sun, is easily identified with the previously discovered Monoceros Ring. Parts of the southern ring at 14 kpc from the Sun (which we call the TriAnd Ring)…
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