IRS/SH surface brightness (10^-12 W cm^-2 sr^-1) maps, corrected for extinction using the extinction law for the local ISM from Chiar & Tielens (2006) and the silicate-based extinction A_V(9.85 μm) (Figs. 8 and 9). The left panels show (from top to bottom) the fine-structure lines [Ne V]14.32 μm, [Ne III]15.55 μm, and [Ne II]12.81 μm. The right panels show (from top to bottom) the [S IV]10.51 μm, [S III]18.71 μm, and [Cl II]14.37 μm lines. The extinction-corrected fluxes and notations are as in Fig. 5.