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Fig. 4

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[Cii] velocity field. The left panel presents the observed data, the central panel the best fit rotating disk model (see Sect. 3.2) and the right panel the residuals. The plus and cross mark the locations of the optical counterpart (Fig. 1) and the [Cii] peak flux (see Table 1), respectively. The observed motions of the [Cii] emission are consistent with a rotating disk model.

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