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Fig. A.1

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Spectra of the 13CS J = 2 − 1 lines. On the x-axis, we show the velocity shift from the systemic velocity VLSR listed in Table 1. In each frame, the red curve represents the best Gaussian fit performed with MADCUBA (see Sect. 2.3). The first column contains the HMSCs, the second the HMPOs, and the third the UCHIIs.
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