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Fig. 7


Azimuthally averaged surface density (top) and midplane temperature (bottom) profiles after 100 binary orbits (6666 years) for radiative models using different initial disk masses. The profiles can be fitted using power-laws when divided into two regimes: An inner region with temperatures of less than about 1000 K and an outer region with temperatures above 1000 K because of a break in the opacity tables at about 1000 K. The inner region follows Σ ∝ r − 1.49  to   −1.51 and T ∝ r − 0.53  to   −0.54, whereas the outer region follows Σ ∝ r − 0.82  to   −1.67 and T ∝ r − 1.39  to   −1.58 for all models.

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