Fig. B.3
Similar to Figs. 2, 5 and B.1, but for simulation D, which has a 20 μG interstellar magnetic field The shocked wind bubble is highly asymmetric from the earliest stages of the evolution and stops expanding in the direction perpendicular to the magnetic field after it reaches approximately 7 pc. The elongated shape of the bubble strongly influences the development of the WR nebula (right panel).
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