Faber-Jackson relation for the subcomponents in NGC 3311 (orange squares) using the V-band photometric model and the velocity dispersion from the finite mixture model. Blue circles indicate the galaxies in the Carnegie-Irvine Galaxy Survey (Ho et al. 2011), while the green lines indicate the results from the SAURON survey (Falcón-Barroso et al. 2011b), including all galaxies (solid line) and slow rotators (dashed line) only.