Warped disk evolution in grid-based simulations | Astronomy & Astrophysics (A&A)

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Fig. C.1

Internal torques G_x, G_Y and G_Z at time t = 120 yr in units of $g_{0} = Ω^{2} r Σ h_{p}^{2}$ $\[g_0=\Omega^2 r \Sigma h_p^2\]$ . Solid lines: From the 3D model. Dashed lines: From the 1D model dwarpy.

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