Line-of-sight velocity, v, velocity dispersion, σ_v, and the v/σ_v ratio as a function of scaled radius in remnant stellar disks after both a single and two consecutive dissipative minor mergers. The same data are also shown for the initial stellar disks, before merging. The gas mass fraction of the merging galaxies increases from the left to the right, from 0 for the S0 case, to 0.2 for the Sbs.