Cosmological hydrodynamical simulations predict that UV diversity in Little Red Dots encodes direct-collapse black hole ages via a rapid transition from BH- to stellar-dominated emission after ~30 Myr.
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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.
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Ultraviolet diversity of Little Red Dots as a probe for direct-collapse black hole ages
Cosmological hydrodynamical simulations predict that UV diversity in Little Red Dots encodes direct-collapse black hole ages via a rapid transition from BH- to stellar-dominated emission after ~30 Myr.
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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.