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- W2398920572 abstract "The processes mainly reviewed are grain evaporation and condensation, grain-grain coagulation, grain diffusion, sedimentation and radial drifts, as well as self-gravitational fragmentation of dust disks. All this is done within the framework of a turbulent prototellar accretion disk. It is shown that such a model can in principle be consistent with a number of cosmochemical observations. However, steady turbulent disks probably do not allow effective grain sedimentation due to losses by radial drifts. An intermittent turbulence is suggested to allow the formation of large seed bodies onto which the disk material can accrete to form planetesimals." @default.
- W2398920572 created "2016-06-24" @default.
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- W2398920572 date "1982-01-01" @default.
- W2398920572 modified "2023-09-23" @default.
- W2398920572 title "Physical Processes of Relevance to the Formation of the Planetary System" @default.
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- W2398920572 doi "https://doi.org/10.1007/978-94-009-7846-1_62" @default.
- W2398920572 hasPublicationYear "1982" @default.
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