Chemical evolution of Mn in the solar neighborhood, as predicted by OMEGA+ (lines, Sect. 5) and derived from stellar spectroscopy (dots, Battistini & Bensby 2015). All predictions include the contribution of Type Ia and CC SNe, using the massive star yields of Limongi & Chieffi (2018, LC18) and Nomoto et al. (2013, N13) for the top and bottom panels, respectively. In each panel the three blue lines show our predictions when we assume that all SNe Ia eject the yields of a given metallicity. The orange line shows our prediction when adopting our metallicity-dependent SN Ia yields. The gray line shows the metallicity-dependent case, but when SNe Ia are assumed to only eject Fe, without Mn, while CC SNe still eject both Fe and Mn.