An analytical ab initio model predicts formation of ultra-faint dwarfs, old globular clusters, and Population III star clusters in early low-mass halos, with properties and abundances matching observations for chosen Pop III masses.
Monthly Notices of the Royal Astronomical Society, 431(4), 3087–3102
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Starbursts at Cosmic Dawn: Formation of Globular Clusters, Ultra-Faint Dwarfs, and Population III star clusters at z > 6
An analytical ab initio model predicts formation of ultra-faint dwarfs, old globular clusters, and Population III star clusters in early low-mass halos, with properties and abundances matching observations for chosen Pop III masses.