Spectrum of the diffuse emission surrounding WR6. Top-left: <mono>tbabs* (vapec+vapec)</mono>, top-right: <mono>tbabs* (vpshock+vpshock)</mono> with fixed abundances, bottom: <mono>tbabs*(vpshock+vpshock)</mono> with the abundances left free to vary, as described in the text. For all the plots, the source model is shown as two red lines (two components). The other dash-dotted lines represent the background, demonstrating that the flat powerlaw is the most significant component of the particle background, while the two thermal dashdot components represent the galactic halo. Finally, the powerlaw shows the unresolved Cosmic X-ray Background. The orange line is the combined model. The models displayed are extracted from the median values of the last 2000 steps of the chain run of <mono>emceee</mono>. The spectra have also been rebinned for a clearer presentation.