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Fig. 7


The gas density in case E simulation of Wareing et al. (2007a) (corresponding to v∗,SM = 125 km s-1, nH = 2 cm-3, and a mass-loss rate of 5 × 10-6 M yr-1), which reveal the formation of vortices in the wake of the AGB star. This stage corresponds to the end of the AGB phase, and resembles the X Her nebula (compare with Fig. 6, remembering that the viewing angle is different, since the space motion of X Her is inclined by 55° with respect to the plane of the sky). Reprinted from Wareing et al. 2007, MNRAS, 382, 1233, with permission from John Wiley & Sons.

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