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Fig. 3


GALEX far UV image of Mira obtained by Martin et al. (2007) overplotted with contours of the Herschel 70 μm image, the thick blue contour corresponding to an IR flux just 3σ above background. The bright white regions correspond to strong UV emission at both ends of the fast jet. Note the absence of IR emission at the end of the southern jet. The red arrow indicates the position of the star in 500 yrs. The bow shock is the faint structure in the background in the south-west.

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