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Fig. 4

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Lorentz factor dependence on the normalized amplitude of the stellar oscillations K for the mode of oscillations (l,m) = (1,1) with θ = 2°, Θ0 = 3°, γ = 1.015, and B0 = 1.0 × 1012   G. The two top panels correspond to the case , while the two bottom panels correspond to the case . The left panels show the solution for φ = 0, the right panels for φ = π.

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