Fig. 13

Top panel: binned and stretched Hα image from the Mayall telescope where the jet-like feature is clearly visible to the NE, while the surrounding planetary nebula can also be seen. Bottom panel: WISE band 3 (resolution = 6.5′′) illustrates the IR emitting material with which the optical shell is recombining. Strong outflow in the polar directions derived from the model presented here can also be seen.
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