NEFERTITI simulations show that the Milky Way's most metal-poor stars largely come from a handful of accreted massive dwarf galaxies, while reproducing the JWST Hebe galaxy at z~11 as a pure Population III system.
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Low-angular-momentum test-particle models of HVCs originating at tens of kpc in a rotating halo reproduce observed kinematics and imply an accretion rate of several solar masses per year sufficient for long-term star formation.
citing papers explorer
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NEFERTITI: Linking early galaxy formation to the assembly of the Milky Way
NEFERTITI simulations show that the Milky Way's most metal-poor stars largely come from a handful of accreted massive dwarf galaxies, while reproducing the JWST Hebe galaxy at z~11 as a pure Population III system.
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Modeling the Accretion of High-Velocity Clouds from a Rotating Halo
Low-angular-momentum test-particle models of HVCs originating at tens of kpc in a rotating halo reproduce observed kinematics and imply an accretion rate of several solar masses per year sufficient for long-term star formation.