Fig. 11
Line profiles of CO and isotopologues from the typical disk with different values of βmid (dashed lines), from the disk model without turbulence (continuous black lines), and from the model with a constant turbulent width of 0.05, 0.1, and 0.2 km s−1 (dotted lines). The disk is seen with an inclination of 45° (0° means that the disk is seen face-on).
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