Fig. 12

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Moment-8 PV diagram of the DCN(3–2) line emission along the plane of the disk (PA=53°). The offset is relative to the phase center of the observations. The black and white points mark the emission peaks obtained by fitting a Gaussian to the emission, respectively, for fixed offset and fixed velocity. The solid squares indicate the points selected by us to define the velocity–radius relation in the Keplerian disk.
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