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Fig. 6


Lorentz factor as a function of radial distance and azimuthal angle φ for a model with stellar oscillations K = 0.02, (l,m) = (1,1), θ = 2°, Θ0 = 3°, γ = 1.015, and B0 = 1.0 × 1012   G. Left panel: . Right panel: .

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