Left panel: σ_{[ OIII ]}/σ_⋆ in the SFR-M_⋆ plane. At high stellar mass, the gas kinematics follows the velocity dispersion of the stellar component. Central panel: B/T median values in the SFR-M_⋆ diagram. The bulge-disk decomposition is taken from the Simard et al. (2011) catalog. We use the values calculated with the r filter. Right panel: σ_⋆ distribution in the SFR-M_⋆ plane. At low stellar masses the σ_⋆ is below to the instrumental resolution. In all panels, the white line shows the mode and dispersion of the MS.