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Fig. E.1


ALMA observations of the HC3N emission at 354.69 GHz (in grey scale, see Wright & Plambeck 2017) overlaid with the emission of acetic acid (purple contours, top panel), aGg–ethylene glycol (cyan contours, middle panel) and gGg–ethylene glycol (green contours, bottom panel). The ALMA synthesized beams are shown as the black circles for the HC3N data (Wright & Plambeck 2017) and as colored ellipses for our data.

This figure is made of several images, please see below:

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