Why Baryons Matter: The Kinematics of Dwarf Spheroidal Satellites
Alyson M. Brooks, Adi Zolotov

TL;DR
This paper demonstrates through high-resolution simulations that baryonic physics significantly alters the dark matter distribution in dwarf spheroidal satellites, aligning theoretical predictions with observed galaxy dynamics.
Contribution
It shows that including baryonic effects in simulations resolves discrepancies between Cold Dark Matter models and observed satellite galaxy kinematics.
Findings
Baryonic feedback reduces dark matter mass in satellite centers.
Simulated satellites match observed velocity and luminosity functions.
Field dwarfs should have higher velocities than satellites at similar luminosities.
Abstract
We use high resolution cosmological simulations of Milky Way-mass galaxies that include both baryons and dark matter to show that baryonic physics (energetic feedback from supernovae and subsequent tidal stripping) significantly reduces the dark matter mass in the central regions of luminous satellite galaxies. The reduced central masses of the simulated satellites reproduce the observed internal dynamics of Milky Way and M31 satellites as a function of luminosity. We use these realistic satellites to update predictions for the observed velocity and luminosity functions of satellites around Milky Way-mass galaxies when baryonic effects are accounted for. We also predict that field dwarf galaxies in the same luminosity range as the Milky Way classical satellites should not exhibit velocities as low as the satellites, since the field dwarfs do not experience tidal stripping. Additionally,…
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