Figure 6.
Surface density profiles of an evolving protoplanetary disc around a 0.1|$\, {\rm M}_{\odot }$| star undergoing Inside-Out with Continued Accretion (IO-A) evolution throughout the disc lifetime. The uppermost blue line shows the initial disc profile, while the black line shows the last disc output before the disc had fully dispersed. The surface density is shown in intervals of intervals of 0.05 Myr.