Same as Fig. 2 for the 2.0 M_⊙ star computed for different initial rotation velocities, as indicated. The mass fractions are multiplied by 100 for ³He, ¹²C, and ¹⁴N, by 2500 for ¹³C, by 50, 1100, and 5 × 10⁴ for ¹⁶O, ¹⁷O, and ¹⁸O respectively, and by 1500 for ²³Na. The vertical arrows show, in all cases, the maximum depth reached by the convective envelope at its maximum extent during the first dredge-up.