Title: The formation of dwarf spheroidal galaxies

Abstract:
We study numerically the formation of dSph galaxies. Intense star bursts, e.g. in gas-rich environments, typically produce a 
few to a few hundred young star clusters, within a region of just a few hundred pc. The dynamical evolution of these star 
clusters may explain the formation of the luminous component of dwarf spheroidal galaxies (dSph). Here we perform a 
numerical experiment to show that the evolution of star clusters complexes in dark matter haloes can explain the formation 
of the luminous components of dSph galaxies.