Fig. 4.
Fraction of the angular momentum flux retained in the super-Eddington disc lin/l0 as a function of the fraction of mass reaching the magnetosphere. The dotted black line corresponds to equal ratios (lin/l0 = Ṁin/Ṁ0, as expected if the net angular momentum is constant); the solid green line corresponds to the expected scaling of a growing spherization radius (Eq. (26)).
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