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The shaping of planetary nebula Sh 2-188 through interaction with the interstellar medium

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Figure

Table 1. Estimates of the distance to, radius of and age of Sh 2−188.
Fig. 3 shows an artificial combination of two three-colour images
Figure 3. An artificial combination of Figs 1 and 2 showing the detail in the bright arc and the faint structure (with some blurring to allow combination ofthe images)
Figure 4. Shown on the left-hand panel is a slice through the data cube showing the logarithm of density at a point 1000 yr into the PN phase
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