Fig. 1

Top panel: histogram of the projected rotational velocities of the new variability class candidates in NGC 3766, divided into candidates with their dominant photometric period P1 > 0.55 d (135° and vertical shaded blue) and P1 < 0.55 d (45° shaded green). Confirmed binaries are vertically shaded. Bottom panel: same as top panel, except for the SPB candidates (45° shaded red) and the hybrid star (135° shaded magenta).
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