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Low levels of methanol deuteration in the high-mass star-forming region NGC 6334I

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Figure

Fig. 1: Velocity integrated intensity map of the 13 CH 3 OH transition at 303.692 GHz with the 1 mm continuum image overlaid in black contours (levels are [10, 20, 40, 80, 160]σ with σ =0.02 Jy/beam)
Table 2: Summary of detected lines
Fig. 6: Column density ratio of CH 2 DOH /CH 3 OH (green) and CH 3 OD /CH 3 OH (blue) for NGC 6334I and other objects
Fig. 7: Column density ratio as function of excitation tempera- tempera-ture. Ratios are normalised to the value derived for T ex = 200 K
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