Fig. 10
Red and black error bars: major-axis projected positions and VLSR (together with the corresponding errors), respectively, for the highest-velocity emission peaks of the six CH3 OH lines with 20 K ≤ Eu ≤ 150 K listed in Table 2. The blue curve is the best Keplerian fit to the data. The horizontal and vertical dashed lines indicate the fitted YSO VLSR and position, respectively.
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