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Fig. 4
Height-dependence of the stellar eccentricity distribution in a cylindrical shell with 2 ≤ R/Rd ≤ 3, for a direct (top row) and a retrograde (bottom row) 1:10 merger, with fgas = 20%. In each panel, the histograms correspond to different heights z above and below the galaxy mid-plane as indicated in the legend.
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