The survivorship bias of protoplanetary disc populations - Internal photoevaporation causes an apparent increase in the median total disc mass with time

Open Access

Fig. 8

Population in the $\dot{M} - M$ $\dot M - M$ plane at 3 Myr, compared to the viscous isochrone. Blue diamonds represent discs that are not dispersed at 4 Myr, while grey crosses represent discs that are dispersed at 4 Myr. The former correspond to the shaded histogram in Fig. 7.

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