Angular-momentum profiles in HH 212, HH 211, and B335 match inside-out collapse with approximate specific-angular-momentum conservation, and B335’s small disk follows from its lower initial j.
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Angular Momentum Evolution from Core to Disk Scales in the Early Phase of Star Formation: Constraints from HH 212, HH 211, and B335
Angular-momentum profiles in HH 212, HH 211, and B335 match inside-out collapse with approximate specific-angular-momentum conservation, and B335’s small disk follows from its lower initial j.