Saturation mechanism and generated viscosity in gravito-turbulent accretion disks

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Fig. 12.

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Toomre parameter at turbulent saturation ⟨Q⟩ plotted as a function of irradiation equilibrium Q₀. Crosses: values derived from simulations by averaging the turbulent state over both box and time according to Eq. (35). Solid line: analytical prediction via Eqs. (36) and (37).

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