Dark Matter Substructure and Dwarf Galactic Satellites

<table>The mass within central 300 pc versus the total virial mass of an NFW halo predicted using the concentration mass relation <svg height="16.4" id="M191" style="vertical-align:-3.38113pt" version="1.1" viewbox="0 0 49.912498 16.4" width="49.912498" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
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</svg> at different redshifts in the concordance WMAP 5-year best fit cosmology. The horizontal dotted lines indicate the range of <svg height="11.9625" id="M192" style="vertical-align:-3.3907pt" version="1.1" viewbox="0 0 28.299999 11.9625" width="28.299999" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
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</svg> masses measured for the Milky Way dwarf satellites.</table>

Advances in Astronomy

Dark Matter Substructure and Dwarf Galactic Satellites

Figure 9