Electron temperatures (T_e) from [S iii] and corresponding sulfur abundances in the WR region. Top left: flux map of nebular [S iii](λ9069). Top right: flux map of auroral [S iii](λ6312). Both flux maps are in units of 10^-17 erg cm^-2 s^-1. Bottom left: electron temperatures from [S iii]. Bottom right: 12 + log (S / H) as derived from T_e. The solar abundance [O/S] is 1.57 (Asplund et al. 2009), so the 12 + log (S / H) scale corresponds to 12 + log (O / H) = 8.2 to 8.4. All panels are approximately 6′′ by 6′′, or 1 kpc by 1 kpc.