Dark Matter Substructure and Dwarf Galactic Satellites
Figure 13
The cumulative radial distribution of the observed “classical’’ Milky Way satellites (solid points connected by the solid line) within 280 kpc and satellites with similar luminosities and within the same distance from their host halo in the model of (4) (dashed lines). The figure also shows the cumulative distribution of all subhalos selected using their current (dotted lines).
