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Fig. 13


3D results for simulation D1, showing the circumstellar density after 40 000 (left and centre) and 300 000 years (right), respectively. The centre panel shows a slice through the 3D data-cube that can be compared directly to the left panel of Fig. 4. Although the shell is not as well resolved as for the 2.5D models, both the eye-like shape and the collimated flows are clearly visible. This confirms the validity of the 2.5D models.

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