Dwarf Galaxies in Voids: Dark Matter Halos and Gas Cooling
Figure 3
(a) Evolution of the characteristic mass of the baryon fraction in distinct haloes (squares) and in newly accreted matter (circles). For comparison the mass accretion histories of five haloes, as depicted in Figure 1, are shown. (b) Evolution of the characteristic circular velocity in distinct haloes and in newly accreted matter. Additionally, the circular velocity histories of the haloes in the left panel is shown.
