Star formation rates for model A with Rg = 2Rd: in isolation (black) and experiencing a 1:5 merger with a high concentration, c = 25, satellite on a planar orbit: radial with first pericenter within the stellar disk (blue), less radial with first pericenter just outside the stellar disk (light green), and even less radial with rperi ≈ 20 kpc (red). A number pericentric passages of the satellite during the different simulations are indicated by the arrows at the top of the figure.
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