Left: projected rotational velocities (v sin i) vs. rotation-corrected gravities (log g_c) for our sample, grouped according to helium abundance. Theoretical predictions for the LMC from Brott et al. (2011) are shown in grey (for three initial masses and two initial rotational velocities as indicated). Predictions for solar metallicity and an initial v_ini of 40% the critical velocity from Ekström et al. (2012) are shown in blue. Right: v sin i distributions for three ranges of gravity: (1) low (log g_c < 3.9); (2) intermediate (3.9 ≤ log g_c ≤ 4.1); and (3) high (log g_c > 4.1).