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Fig. 4.

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Density contour, magnetic streamlines, and flow streamlines for an expanding galactic bubble with a large-scale magnetic field with a thick galactic disk at the left (B = 10−4 Gauss) and the right (B = 10−2 Gauss) at t = 10 Myr. Left: density contour showing variations in density and the magnetic streamlines representing the direction and strength of the magnetic field, color-coded to indicate their emergence zone. Right: flow streamlines indicating the motion of matter, also color-coded to indicate their emergence zone.

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