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- W2079721887 abstract "We examine the consequences of a model for the circulation of solids in a protoplanetary nebula in which aerodynamic drag is counterbalanced by the recycling of material to the outer disc by a protostellar outflow or a disc wind. This population of circulating dust eventually becomes unstable to the formation of planetesimals by gravitational instability, and results in the ultimate deposition of 30--50 earth masses in planetesimals on scales R< 1 AU. Such a model may provide an appropriate justification for the approximately power law initial conditions needed to reproduce observed planetary systems by in situ assembly." @default.
- W2079721887 created "2016-06-24" @default.
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- W2079721887 date "2014-04-17" @default.
- W2079721887 modified "2023-09-26" @default.
- W2079721887 title "The circulation of dust in protoplanetary discs and the initial conditions of planet formation" @default.
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- W2079721887 doi "https://doi.org/10.1093/mnras/stu471" @default.
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