Cosmological zoom-in simulations reproduce the Milky Way's three kinematic phases and tie transitions to cool gas conversion rates, baryonic sloshing, and circumgalactic medium virialization.
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From protogalaxy through thick and thin: Why did the Milky Way evolve in three kinematic phases?
Cosmological zoom-in simulations reproduce the Milky Way's three kinematic phases and tie transitions to cool gas conversion rates, baryonic sloshing, and circumgalactic medium virialization.