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Fig. 12


Star formation rates for models C and D with Rg = Rd, fgas = 0.9, z0 = 0.3Rd, and a dark matter halo concentration of either c = 5 (C3 and D2) or c = 15 (C1 and D1), during the 1:5 merger with a satellite on a prograde orbit with an inclination with the plane of the disk of 0 (for models C) or 30 degrees (for models D). 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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