Slices of density (first column), pressure (second column), radial velocity (third column), and azimuthal velocity (fourth panel) of the bound remnant 1000 s after the explosion. The top row shows slices in the plane of rotation of the initial binary system; the bottom row shows slices that are perpendicular to it. The velocities are relative to the rest frame velocity of the bound remnant. The inner part of the 0.16 M_⊙ bound remnant is essentially spherical, while the outer parts are clearly not.