Abstract
AbstractIt is the aim of our letter to embedd the presently well understood scale of stellar mass into a simple cosmological scenario for the origin of Population III objects. The result of our consideration will be that if the first bound objects with typical stellar mass of the order of 30 M⊙ could evolve as ordinary stars ending up exploding (Type II supernovae) the problem of the pregalactic enrichment of a primordial gas cloud be solved.
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