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Fig. B.1

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Channel maps of the [C I] J = 1−0 emission of the non-Keplerian redshifted component in DO Tau. Channel velocities are relative to the cloud velocity. The white ellipse denotes the best-fit ellipse to the pole-on outflow observed in CO (Bmaj = 3″, Bmin = 2″, PA = 167°; Fernández-López et al. 2020). The arc-like emission is striking similar to the pole-on outflow observed in CO.

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