Azimuthally averaged surface density (top) and eccentricity (bottom) for locally isothermal disks, with H/r = 0.05, around the two systems, Kepler-34 and Kepler-38. The figure shows the profiles for the final equilibrium state without any embedded planet. The radial coordinate has been scaled by the binary separation which is 0.23 AU for Kepler-34 and 0.15 AU for Kepler-38. The results for Kepler-38 have been taken from Kley & Haghighipour (2014).