Fig. C.1

Schematic illustration of the disk-envelope model employed here and by T13. The material inside the centrifugal radius, RC, rotates with Keplerian velocity (solid arrow), while the material outside RC is rotating and infalling (dashed arrows). The blue- and redshifted material is shown in blue and red, respectively. The system is 5° inclinded from edge-on, such that the disk and envelope west of the protostar are nearest to the observer.
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