Abstract:
:Discs of gas and dust around million-year-old stars are a by-product of the star formation process and provide the raw material to form planets. Hence, their evolution and dispersal directly impact what type of planets can form and affect the final architecture of planetary systems. Here, we review empirical constraints on disc evolution and dispersal with special emphasis on transition discs, a subset of discs that appear to be caught in the act of clearing out planet-forming material. Along with observations, we summarize theoretical models that build our physical understanding of how discs evolve and disperse and discuss their significance in the context of the formation and evolution of planetary systems. By confronting theoretical predictions with observations, we also identify the most promising areas for future progress.
journal_name
R Soc Open Scijournal_title
Royal Society open scienceauthors
Ercolano B,Pascucci Idoi
10.1098/rsos.170114subject
Has Abstractpub_date
2017-04-26 00:00:00pages
170114issue
4issn
2054-5703pii
rsos170114journal_volume
4pub_type
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