Inferring the physics of protoplanetary disc evolution from the irradiated Cygnus OB2 region - A comparison of viscous and MHD wind-driven scenarios

Open Access

Fig. 8

Stellar mass dependence of the disc radii from our fiducial populations with $ℱ_{10 G_{0}}$ ${{\cal F}_{10{{\rm{G}}_0}}}$ (see Table 1), shown at 3 Myr. The markers indicate the 25th and 75th percentiles. The observational trend (black line) is shown along a 0.5 and 1 dex spread around the mean (Andrews 2020).

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