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Fig. 8

image

13CO (horizontal axis) and C18O (verticalaxis) line luminosities from the physical–chemical models of protoplanetary disks (color dots) by Miotello et al. (2016) overlaid on the measured line luminosities from the velocity-aligned stacking method (data points with error bars). The C18O non-detected disks are presented with open circles. Red, orange, yellow, green, blue, purple, and gray dots denote the models with disk masses of 10−1, 10−2, 5 × 10−3, 10−3, 5 × 10−4, and 10−5, 10−4 M.

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