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Fig. 9.

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Vertical velocity and mass flux of hot H2 along the redshifted lobe of DG Tau B. (a) Vz as a function of deprojected distance Z from the source, derived from H2 1−0 S(1) SINFONI/VLT observations. For comparison, the shaded red area shows the range of Vz across the CO redshifted conical flow, from outer to inner streamlines DV20. (b) Mass flux of hot H2 as a function of Z (see text).

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