Atomic hydrogen shielding of Lyman-Werner radiation increases final Population III stellar masses by ~22% and keeps the HII region confined near the protostar in radiation-MHD simulations.
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Radiative Feedback in Population III Protostellar Growth: HI Shielding \& HII Region Trapping
Atomic hydrogen shielding of Lyman-Werner radiation increases final Population III stellar masses by ~22% and keeps the HII region confined near the protostar in radiation-MHD simulations.