Fig. G.1

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Position-velocity diagram of the ALMA C18O datacube, centered at the position of the protostar, with a PA of 157°.1 and a width of 0″.4. The black curves show the Keplerian rotation profile produced by three protostellar massses: the dotted line shows the Keplerian curve for a protostar of 0.1 M⊙ (Brassfield & Bourke 2011), the dashed line for 0.2 M⊙, and the dash-dotted line for 0.3 M⊙. The dotted horizontal line marks the protostar’s vlsr = 10.2 km s−1. The scalebar represents one beam width (120 au or 0″.4)
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