Photoevaporation of protoplanetary discs – 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 he...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2006-06, Vol.369 (1), p.229-239 |
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