The UV view of multi spin galaxies: insight from SPH simulations
  The UV images of GALEX revealed that ~30% of Early Type Galaxies (ETG) show
UV emission indicating a rejuvenation episode. In ETGs with multiple spin
components this percentage increases at 50%. We present here the
characteristics of this sample and our smooth particle hydrodynamic (SPH)
simulations with chemo-photometric implementation that provide dynamical and
morphological information together with the spectral energy distribution (SED)
at each evolutionary stage. We show our match of the global properties of two
ETGs (e.g. NGC 3626 and NGC 5173). For these galaxies we can trace their
evolutionary path.
