Back-calculated initial masses of Galactic globular clusters show the pristine-star fraction versus mass relation is tighter for disk-born clusters than for accreted groups, and generalizes the fixed 2P-star formation threshold to a fitted power law.
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Cracking the relation between mass and 1P-star fraction of globular clusters: III. Initial distributions of in-situ and ex-situ clusters
Back-calculated initial masses of Galactic globular clusters show the pristine-star fraction versus mass relation is tighter for disk-born clusters than for accreted groups, and generalizes the fixed 2P-star formation threshold to a fitted power law.