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Fig. 5


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

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