A theoretical explanation for the Central Molecular Zone asymmetry
Mattia C. Sormani, Robin G. Tress, Matthew Ridley, Simon C.O. Glover,, Ralf S. Klessen, James Binney, John Magorrian, Rowan Smith

TL;DR
This paper explains the long-standing asymmetry in the Milky Way's Central Molecular Zone as a transient phenomenon caused by hydrodynamical and thermal instabilities in gas flow within a barred galaxy potential, supported by high-resolution simulations.
Contribution
It provides a novel theoretical explanation for the CMZ asymmetry using 3D hydrodynamical simulations that incorporate chemical networks, highlighting the role of instabilities in creating transient asymmetries.
Findings
Asymmetry arises spontaneously from instabilities despite symmetric initial conditions.
The asymmetry is transient and can reverse over tens of megayears.
Simulations show fluctuations matching observed asymmetry levels over time.
Abstract
It has been known for more than thirty years that the distribution of molecular gas in the innermost 300 parsecs of the Milky Way, the Central Molecular Zone, is strongly asymmetric. Indeed, approximately three quarters of molecular emission comes from positive longitudes, and only one quarter from negative longitudes. However, despite much theoretical effort, the origin of this asymmetry has remained a mystery. Here we show that the asymmetry can be neatly explained by unsteady flow of gas in a barred potential. We use high-resolution 3D hydrodynamical simulations coupled to a state-of-the-art chemical network. Despite the initial conditions and the bar potential being point-symmetric with respect to the Galactic Centre, asymmetries develop spontaneously due to the combination of a hydrodynamical instability known as the "wiggle instability" and the thermal instability. The observed…
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