CN rings in full protoplanetary disks around young stars as probes of disk structure

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Fig. 15

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Comparison between CN, ¹³CO and C¹⁸O integrated flux dependence on the total disk mass. The ¹³CO and C¹⁸O fluxes are taken from Miotello et al. (2017). The solid lines represent the fit functions of the median for ¹³CO (red) and C¹⁸O (blue).

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