Simulations find that post-reionization star formation in dwarf galaxies correlates with higher metallicity, rounder stellar distributions, and rounder inner dark matter halos, while quenched relics show the opposite.
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Co-evolution of baryons and dark matter halos of LYRA dwarf galaxies
Simulations find that post-reionization star formation in dwarf galaxies correlates with higher metallicity, rounder stellar distributions, and rounder inner dark matter halos, while quenched relics show the opposite.