Fitting results for NGC 884 using isochrone-clouds with Z = 0.014, leading to age of ∼11 Myr. Left: same as left panel of Fig. 6. Upper, middle and lower panel of central plots: v sin i, the dominant oscillation frequency and its amplitude vs. fractional core mass. Right: same as right panel of Fig. 6, but blue denotes stars with measured oscillations and red denotes stars with measured v sin i. Pink dotted distribution is for those stars with the minimum amount of mixing.