Figure 1.
Peak brightness images for the lines of CS, CH3OH, HC3N, SiO, HNCO and HOCO+. These are the six lines we observed with the most widespread strong distribution. The grey-scale is peak brightness as $T_{A}^{*}$ in K here and in Figs 2–4.

Peak brightness images for the lines of CS, CH3OH, HC3N, SiO, HNCO and HOCO+. These are the six lines we observed with the most widespread strong distribution. The grey-scale is peak brightness as |$T_{A}^{*}$| in K here and in Figs 2–4.

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