Fig. A.1

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Spectra of CH3CN(5K-4K) for the sources for which at least one transition has been detected. The red line is the synthetic spectrum obtained by the best fit within MADCUBA. For G31.41+0.31, the synthetic spectrum is not reported since the fit does not converge. VLSR of sources G014.99-0.67 and 18445-0222M3 during observations mildly differ from the correct value. VLSR has been corrected after observations, and given in Table 3.
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