The evolution of the water distribution in a viscous protoplanetary disk
Fred J. Ciesla,Jeffrey N. Cuzzi +1 more
TL;DR: In this article, the authors present a model which tracks how the distribution of water changes in an evolving disk as the waterbearing species experience condensation, accretion, transport, collisional destruction, and vaporization.
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About: This article is published in Icarus. The article was published on 01 Mar 2006. and is currently open access. The article focuses on the topics: Protoplanetary disk & Planetary migration.
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Citations
Protoplanetary Disks and Their Evolution
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A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution
Steven A. Balbus,John F. Hawley +1 more
TL;DR: In this article, a linear analysis is presented of the instability, which is local and extremely powerful; the maximum growth rate which is of the order of the angular rotation velocity, is independent of the strength of the magnetic field.
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