A fully cosmological model of a Monoceros-like ring
Facundo A. G\'omez, Simon D. M. White, Federico Marinacci, Colin T., Slater, Robert J. J. Grand, Volker Springel, R\"udiger Pakmor

TL;DR
This study uses a cosmological simulation to model the formation of a Monoceros-like stellar ring, revealing that a minor satellite fly-by can induce large-scale vertical structures in a galactic disk.
Contribution
It demonstrates that a low-mass, low-velocity fly-by can generate Monoceros-like features through halo response, a novel explanation for such structures.
Findings
A Monoceros-like ring can form from halo response to a minor satellite encounter.
The pattern originated as an $m=1$ mode and evolved into a spiral.
The satellite's mass is about 5% of the host, with an 80 kpc pericentre and 215 km/s velocity.
Abstract
We study the vertical structure of a stellar disk obtained from a fully cosmological high-resolution hydrodynamical simulation of the formation of a Milky Way-like galaxy. At the present day, the disk's mean vertical height shows a well-defined and strong pattern, with amplitudes as large as 3 kpc in its outer regions. This pattern is the result of a satellite - host halo - disk interaction and reproduces, qualitatively, many of the observable properties of the Monoceros Ring. In particular we find disk material at the distance of Monoceros ( 12-16 kpc, galactocentric) extending far above the mid plane ( 30, 1-2 kpc) in both hemispheres, as well as well-defined arcs of disk material at heliocentric distances kpc. The pattern was first excited Gyr ago as an mode that later winds up into a leading spiral pattern.…
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