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Trapping of H <scp>ii</scp> regions in Population III star formation

Trapping of H <scp>ii</scp> regions in Population III star formation

Radiative feedback from massive Population III (Pop III) stars in the form of ionising and photodissociating photons is widely believed to play a central role in shutting off accretion onto these stars. Understanding whether and how this occurs is vital for predicting the final masses reached by these stars and …