Characteristics of a star with a mass of 16 M_⊙ 5 × 10⁴ years after the end of the common envelope stage for ζ = 0.8. Distributions of the angular velocity of rotation Ω(r) (top), the amplitude of the velocity of the meridional circulation U(r) (middle), and the flux of the angular momentum (bottom): turbulent F_t(r) (solid line), advective F_ad(r) (dashed line), and full F(r) (thick solid line) are shown depending on the average distance to the isobar.