Title:Models of faint galaxy production through star cluster evolution (working title)

Abstract:
The mass-to-light ratios of ultra-faint dwarf galaxies are comparable to a moderate-size star cluster 
embedded in a moderate-mass dark matter halo. We will present N-body models of star clusters evolving 
within dark matter halos that explore this scenario in terms of the dynamics of the system and the final 
observable state, including the possible creation of dark galaxies.