Fig. 20
PV plot of the CH3CN(12–11) K = 2 line emission (colour scale and contours) for G345.49 M. The cut is made through the strongest continuum peak, along PA = 15°. Unlike the PV plots of the other sources, here we do not plot the 13CH3CN(13–12) emission since it is barely detected (see Fig. 10). The white pattern corresponds to Keplerian rotation about a 10 M⊙ star.
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