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Fig. B.1.

Inviscid radial circulation velocity magnitudes, Uk(r) plotted as a function of normalised radius for an n = 3 polytrope with M = 3 M⊙, R = 1.75 R⊙, L = 93 L⊙ and a companion mass of M = 3 M⊙. The ratio of stellar radius to orbital separation is set to be 0.35, representing a near-contact system.
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