The evolution of dust in discs influenced by external photoevaporation
Monthly Notices of the Royal Astronomical Society(2020)
Abstract
Protoplanetary discs form and evolve in a wide variety of stellar environments and are accordingly exposed to a wide range of ambient far-ultraviolet (FUV) field strengths. Strong FUV fields are known to drive vigorous gaseous flows from the outer disc. In this paper we conduct the first systematic exploration of the evolution of the solid component of discs subject to external photoevaporation. W...
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Key words
planets and satellites: formation,protoplanetary discs,submillimetre: planetary systems
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