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Fig. 23.

image

Radial abundance gradient measured in dex/Re, d (left column panels) and dex/Re, g (right column panels). Row a panels: radial abundance gradient as a function of the rotation velocity Vrot, row b panels: as a function of the stellar mass Msp, row c panels: as a function of galaxy luminosity LB, row d panels: as a function of optical radius R25, and row e panels: as a function of the stellar mass Mma. The grey points at each panel are the data for individual MaNGA galaxes from our sample, while the dark points are the binned mean values. The dashed line in the left and right column panels show the mean values of the gradient in units of dex/Re, d and dex/Re, g, respectively.

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