The amplification or dampening of hydrodynamically instable features may be modified by the presence of dust. Also the dynamics of dust will surely follow pressure maxima in a protoplanetary disc. Therefore there is ample potential for complex interactions between the gas and dust material which we aim to study.

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Hydrodynamic vortices as dust traps (M.Sc project).

Mean Gas opacities for circumstellar environments (PhD Project).

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