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Fig. 5.
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Variation in ℐKr(r) with s computed for the (ℓ,m) = (1, −1) modes in the case of a uniform radial field (which implies that ℐKr(r) = ℐ) and for a M = 1.6 M⊙, R = 2.13 R⊙, Xc = 0.35 stellar model.
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