Three-dimensional evolution of radiative circumbinary discs: The size and shape of the inner cavity

Open Access

Fig. 10

For Kepler-34, 2D surface density distributions for the 2D and 3D models and for different α parameter values. These snapshots correspond to a simulated time of 2000 T_bin for calculations with α = 10⁻³–10⁻², and of 1500 T_bin for the run with α = 0.1.

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