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Fig. 3.

image

Angular velocity of rotation in the star’s interior Ω(m) during the common envelope stage and after its completion. The angular velocity distribution is shown for ζ = 0.8 (top line), ζ = 0.5 (middle line), and ζ = 0.2 (bottom line) for the following time instants during the common envelope stage (left panel): 1 year (solid line), 10 years (dashed line), 30 years (dash-dotted line), and 100 years (thick solid line). The time instants after its completion (right panel) are 103 years (thick solid line), 5 × 103 years (solid line), 104 years (dashed line), and 5 × 104 years (dash-dotted line).

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