Abstract
We performed smooth particle hydrodynamic (SPH) simulations including star formation and self-consistent chemo-photometric evolutionary population synthesis (EPS) predictions from far-UV to 1 mm, of isolated collapsing triaxial systems. The dependence of the system evolution on some parameters so far unexplored, such as the total mass, initial geometry, dynamical state of the collapsing halo and the effects of different baryonic to dark matter (DM) mass ratios has been investigated. We find important connections between dark and luminous matter.
