Coexistence of coagulation and streaming instabilities in protoplanetary disks

Open Access

Fig. 2

Case of ϵ = 0.02, snapshots of the dust density (left) and Stokes number (right) for model E0v02S0v01c with St = 0.01 (left) and for model E0v02S0v1c with St = 0.1 (right). Both models include the effect of coagulation and result in the growth of the CI.

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