L. Tornatore, Andrea Ferrara, Raffaella Schneider
Abstract
The physical conditions in primordial star-forming regions appear to systematically favor the formation of very massive stars. This is due to the combined effect of the larger gas fragmentation scale and accretion rate, and the very
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The physical conditions in primordial star-forming regions appear to systematically favor the formation of very massive stars. This is due to the combined effect of the larger gas fragmentation scale and accretion rate, and the very
Key concepts: Metallicity, Physics, Stars, Star formation, Astrophysics, Population, Reionization, Redshift