The Effect of Tidal Stripping on Composite Stellar Populations in Dwarf Spheroidal Galaxies
Figure 7
Projected density (a) and velocity dispersion (b) profiles for satellites evolved in Orb1 and Orb4 for a longer time interval: Gyr, instead of the fiducial Gyr. Notice for Orb4 that, as mass depletion proceeds further, the spatial and kinematical segregation between and is increasingly erased.