Fig. 5
Comparison of Be-type stellar (black/blue) vsini and nitrogen abundances with those of B-type stars (black open circles) from Hunter et al. (2009a) for both metallicity regions analysed (SMC – upper panel, LMC – lower panel). Be-type star abundances are plotted for pre- (blue) and post-contamination (black) correction values. Upper limits are denoted with triangles.
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