Estimated nitrogen abundances and projected rotational velocities plotted for the SMC (top panel) and LMC (bottom panel) Be-type stellar samples before and after contamination correction (blue and black respectively). Simulations are based on the rotational velocity distribution of Hunter et al. with only B-type stars rotating with critical velocity between 65% and 75% as to represent a sample of stars rotating around 70% of critical velocity. Marked on each plot as a black dashed line is the baseline nitrogen abundance. Simulations predict too high nitrogen abundances for the LMC, with a mixed view given for the SMC.