Photoevaporation of protoplanetary discs โ II. Evolutionary models and observable properties
Photoevaporation of protoplanetary discs โ II. Evolutionary models and observable properties
We present a new model for protoplanetary disc evolution. This model combines viscous evolution with photoevaporation of the disc. However, in a companion paper we have shown that at late times such models must consider the effect of stellar radiation directly incident on the inner disc edge, and here we โฆ