Razor-thin dust layers in protoplanetary disks: Limits on the vertical shear instability

Open Access

Fig. 3

For the fiducial model shown in Figs. 1 and 2, the vertical gas velocity v_z at r = r₀ and z = 0 in units of the local isothermal sound speed as a function of time in units of orbits after the 300th orbit.

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