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

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• Barbara Ercolano, LMU Munich
• Thursday 16 January 2020, 16:00-17:00
• Sackler Lecture Theatre, IoA (tea at 3:30 pm).

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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.

This talk is included in these lists:

• Combined External Astrophysics Talks DAMTP
• Cosmology lists
• Cosmology, Astrophysics and General Relativity
• Institute of Astronomy Colloquia
• Institute of Astronomy Talk Lists
• Kavli Institute for Cosmology Talk Lists
• Priscilla
• Sackler Lecture Theatre, IoA (tea at 3:30 pm)

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