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A simple model for the evolution of the dust population in protoplanetary disks
Astronomy and Astrophysics · 2012 · Vol. 539 · pp. A148–A148
T. Birnstiel✉(Excellence Cluster Universe)Hubert Klahr(Max Planck Institute for Astronomy)Barbara Ercolano(Excellence Cluster Universe)
Abstract
Context. The global size and spatial distribution of dust is an important ingredient in the structure and evolution of protoplanetary disks and in the formation of larger bodies, such as planetesimals.
Astrophysics and Star Formation StudiesAstro and Planetary ScienceStellar, planetary, and galactic studiesPlanetesimalContext (archaeology)Protoplanetary diskPhysicsPopulationAstrobiologyAstrophysicsPlanetGeologyPaleontology
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References
Particle stirring in turbulent gas disks: Including orbital oscillations
Icarus · 2007 · 614 citations
Settling and growth of dust particles in a laminar phase of a low-mass solar nebula
Icarus · 1986 · 637 citations
Aerodynamics of solid bodies in the solar nebula
Monthly Notices of the Royal Astronomical Society · 1977 · 1,893 citations
The Evolution of Viscous Discs and the Origin of the Nebular Variables
Monthly Notices of the Royal Astronomical Society · 1974 · 2,513 citations
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