High turbulence in the IM Lup protoplanetary disk - Direct observational constraints from CN and C2H emission

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Fig. 8

Total intrinsic linewidth determined from the best-fit DISCMINER model (solid black line; this is the same as the dashed black line in the bottom-right panel of Fig. 6). It is compared to the thermal component obtained using the ¹³CO (blue) or ¹²CO (orange) brightness temperatures.

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