Strong Lyman-Werner radiation can delay star formation in 10^8-solar-mass halos, enabling Population III starbursts of up to ~10^6 solar masses before internal metal enrichment ends them.
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How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background
Strong Lyman-Werner radiation can delay star formation in 10^8-solar-mass halos, enabling Population III starbursts of up to ~10^6 solar masses before internal metal enrichment ends them.