Early planet formation in embedded protostellar disks - Setting the stage for the first generation of planetesimals

Open Access

Fig. 11

Midplane dust-to-gas ratios for the Ref-med collapse model at the same time steps as shown in Fig. 10. The lines and hashed regions have the same definition as in Fig. 9. The dust-to-gas ratio never exceeds the threshold for the onset of the streaming instability at any of the shown time steps.

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