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Disc-Based Estimation of the Local Dark Matter Density and Velocity Distribution in IllustrisTNG50
astrophysics-of-galaxiescosmology-and-nongalactic-astrophysicshigh-energy-physics-experimenthigh-energy-physics-phenomenology
We study the dark matter (DM) density and velocity distribution in the solar neighborhood of Milky Way-like galaxies using the TNG50-1 run of the IllustrisTNG simulation suite. Milky Way-like galaxies are selected according to both their halo mass and their bulge-to-total stellar mass ratio, and the
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