Fig. 12
The resultant SHAPE model of MyCn 18’s nebular morphology and an HST[N ii]6584 Å image scaled for comparison. Also shown are the long-slit positions used for the observed and synthetic P-V arrays in Fig. 11, labelled 1 (slit 1 down the major-axis) and 2 (slit 2 across the minor-axis). Both slit widths have a value of 0.8 arcsec.
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