Stacked eROSITA spectra of the 96 M dwarf (top row) and the 30 FGK stars (bottom row) in the western Galactic hemisphere and within 10 pc of the Sun (Zheng et al. in prep.). The stack is computed as if all stars were at 10 pc from us. The left column shows the average spectra and the best fit model, composed of two to three thermal components with variable elemental abundances. In contrast, the right column shows the spectra and residuals for a fit with a two-temperature model with abundances fixed at the solar value and the temperatures fixed at 0.2 and 0.7 keV.