Fig. 4.
Surface density distributions of the stellar component viewed edge-on at the time of maximum distortion out of the disk plane. For B2 no clear distortion is detected so the final output of the simulation (t = 3 Gyr) is shown. The surface density was normalized to the central maximum value in each case and the contours are equally spaced in log Σ with Δ log Σ = 0.05.
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