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Fig. 1

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Azimuthally and time-averaged profiles of the disk’s eccentricity (left column) and surface density (Σ, right column) obtained with the series of locally isothermal disk models described in Sect. 3. In the density profile plot we include the initial, unperturbed profile, which is shown as reference. Results are shown at 60 orbits of the secondary, and time-averaging is done over 5 orbits. Several values of the disk’s aspect ratio at 1 AU are considered and two secondary-to-primary mass ratios of q = 0.4 (upper panels) and q = 0.1 (lower panels).

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