The coexistence of the streaming instability and the vertical shear instability in protoplanetary disks : Planetesimal formation thresholds explored in two-dimensional global models
The streaming instability is a promising mechanism to induce the formation of planetesimals. Nonetheless, this process has been found in previous studies to require either a dust-to-gas surface density ratio or a dust size that is enhanced compared to observed values. Employing two-dimensional global simulations of protoplanetary disks, we show that the vertical shear instability and the streaming
