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Fig. 24

image

Synthetic ALMA observation simulation of the Keplerian disk model (with a bipolar outflow) with the C36-1 antenna configuration (res = 1.5′′, LAS = 11′′), for which the original model has been rescaled to a size 3.5 times greater than it was in Fig. 23. The effect of the largest angular scale being exceeded can be seen around zero velocity.

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