Toroidal vortices as a solution to the dust migration problem
Authors:
Loren-Aguilar et al
Abstract:
In an earlier letter, we reported that dust settling in protoplanetary discs may lead to a dynamical dust-gas instability that produces global toroidal vortices. In this letter, we investigate the evolution of a dusty protoplanetary disc with two different dust species (1 mm and 50 cm dust grains), under the presence of the instability. We show how toroidal vortices, triggered by the interaction of mm grains with the gas, stop the radial migration of metre-sized dust, potentially offering a natural and efficient solution to the dust migration problem.
Friday, March 4, 2016
Toroidal Vortices Explain the Dust Migration Problem
Labels:
dust,
protoplanetary disks,
vortices
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