Fig. 4.
Difference in angular velocities of rotation between the convective core and the star’s surface. The ratio of the angular rotational velocities of the convective core and the star’s surface Ωc/Ωs(t) during the common envelope stage (left panel) and after its completion (right panel) is shown for ζ = 0.8 (solid line), ζ = 0.5 (dashed line), and ζ = 0.2 (dash-dotted line).
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