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The dispersal of planet forming discs and its role on the formation and evolution of planets

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The formation and evolution of planets is intimately related to the physical conditions, the evolution and the dispersal of their natal planet forming disc. In this talk I will summarise the basics behind photoevaporation models of disc dispersal, emphasising some of their expected influence on planet formation and migration. I will also focus on the predictive aspects of current models and how well they compare with current observations.

This talk is part of the Institute of Astronomy Colloquia series.

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