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.
year = 2023, month = jun, volume =
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A LambdaCDM black hole growth model predicts that observed high-redshift Little Red Dots are the luminous tip of a larger population undergoing super-Eddington accretion in nuclear bursts.
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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Super-Eddington accretion of black holes in early nuclear bursts gives birth to Little Red Dots
A LambdaCDM black hole growth model predicts that observed high-redshift Little Red Dots are the luminous tip of a larger population undergoing super-Eddington accretion in nuclear bursts.