Spectra of four regions: in the dark lane region (upper left), the small region (upper right), the diffuse region (lower left), and inside of the N11 bubble (lower right). Spectra of all TMs are shown in different colors. The source components are highlighted with thick lines (solid: lower-temperature vapec1; dashed: higher-temperature vapec2). The straight lines show the particle background. The thin dotted lines indicate the spectral components of the astrophysical background spectrum.