Fig. 5.
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Comparison of the characteristics of the Milky Way and galaxies from our sample. Panel a: stellar masses M⋆ as a function of rotation velocity Vrot (Tully–Fisher diagram). The grey points in each panel denote individual MaNGA galaxies, while the goldenrod points correspond to nearby galaxies in our sample. The solid line is the linear fit to all the data, while the dotted lines are ±σ deviations. The red circle marks the position of the Milky Way. Panel b: optical radius R25 as a function of rotation velocity Vrot. Panel c: optical radius R25 as a function of stellar mass M⋆. Panel d: black hole mass MBH as a function of stellar mass M⋆. Panel e: central oxygen abundance (O/H)0 as a function of stellar mass M⋆. Panel f: oxygen abundance at the optical radius (O/H)R25 as a function of stellar mass M⋆.
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