Planetesimal formation via the streaming instability in simulations of infall-dominated young disks

Open Access

Fig. D.3

Same as Fig. D.2, but instead of the temperature the radial profile of the internal torque parameter, α_SS (cf. Eq. 10), is shown, and is scaled linearly if the absolute value is less than 10⁻⁴, but logarithmically otherwise.

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