Fig. 6.
Momentum flux in the star’s interior at the common envelope stage for ζ = 0.8. The turbulent flux Ft (solid line), the advective flux Fad (dashed line), and the total flux F (thick solid line) are shown 30 years after the start of the common envelope stage depending on the mass of the matter inside the isobar (left panel) and the average distance to the isobar (right panel).
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