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Fig. C.3

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Radial velocity υrad maps for the mid-infrared transitions studied in this work. The grey star indicates the position of the protostar. The white circle indicates the PSF FWHM in the channel that contains the wavelength of the transition. Each coloured spaxel corresponds to a Gaussian fit with a peak height larger than 5σ, with σ indicating the uncertainty on the continuum flux as described in Appendix A.

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