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Dissipative phenomena occurring during the orbital evolution of a dwarfsatellite galaxy around a host galaxy may leave signatures in the starformation activity and signatures in the colour magnitude diagram of the galaxystellar content. Our goal is to reach a simple and qualitative description ofthe these complicated phenomena. We develop an analytical and numericaltechnique able to study ram pressure, Kelvin-Helmholtz instability,Rayleigh-Taylor and tidal forces acting on the star formation processes inmolecular clouds. We consider it together with synthetic colour magnitudediagrams techniques. We developed a method to investigate the connectionsexisting between gas consumption processes and star formation processes in thecontext of the two extended-body interaction with special attention to thedwarf galaxies dynamical regime.

Dissipative phenomena in extended-bodies interactions I: Methods Dwarf galaxies of the Local Group and their synthetic CMDs