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Fig. 3.

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Density contour for an expanding galactic bubble in a magnetized halo with a dipolar magnetic field at t = 10 Myr. The galactic wind has a mass flux of = M yr−1. Top panel: B0 = 10−4 Gauss (left) and B0 = 10−5 Gauss (right). Bottom panel: dipole B0 = 10−2 Gauss (left) and B0 = 1 Gauss (right). The isocontour of the density is represented by white, blue and black lines, corresponding to their respective density isocontour values of 5 × 10−26, 5 × 10−26 and 1.2 × 10−25, respectively.

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