Fig. C.2

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Intensity maps of 13CO (2 − 1) emission from IRAM 30-m telescope integrated over the blueshifted and redshifted wings of emission, showing the outflow structure. The position of the strongest source in the field is depicted by a star. The blue and red arrows correspond to the estimated directions of bipolar blueshifted and redshifted molecular outflows, respectively. A scale-bar is shown in the bottom right corner of each panel. The map size of the IRAM 30-m observations is 1.5′ by 1.5′ with a half-power beam width of ~11″ at this frequency.
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