Left panel: electron fraction of the remnant 5 ms after merger in the MC simulation with the highest packet count. Dashed white lines are density contours at ﹩{10}^{\mathrm{9,11,13}}\,{\rm{g}}\,{\mathrm{cm}}^{-3}.﹩ Middle panel: the same, for the M1 simulation. Regions just outside of the neutron star and disk are slightly denser in the MC simulations (possibly due to he higher ν_x luminosity), and matter is more neutron rich in the outflow regions. Right panel: composition of the unbound material. Filled histograms shows the polar outflows only.