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ionized outflow originates from disk radii r ≤ 1015 cm inside of which ly-continuum photons from the protostellar accretion shock are intercepted.
l'écoulement ionisé provient de disques de rayons r ≤ 1015 cm à l'intérieur desquels les photons du continuum ly provenant du choc de l'accrétion protostellaire sont interceptés.