Left panel: specific stellar angular momentum-stellar mass relation (Fall relation) for a sample of 92 nearby disc galaxy. Each galaxy is represented by a circle coloured by Hubble type. The black dashed line is the best-fitting linear model and the grey band is the 1σ orthogonal intrinsic scatter. Bottom panel: orthogonal residuals around the linear model. Right panel: as in the left panel, but for the discs only (i.e. after removing the contribution from the bulges).