scale, in order to bring out the often faint structural features of the nebulae. In spite of the generally low signal-to-noise (S/N) ratio in the [*HST*]{} images (which, after all, were not obtained for this purpose), we were able to confirm several of the objects as genuine PNe. Furthermore the 01 resolution of the [*HST*]{} images permits a solid morphological classification to be assigned, which is not possible from the @RP06b data. The morphological classifications would ordinarily be based on the appearance of the nebula in the monochromatic light of either \[\] $\lambda5007$ or H$\alpha$ (possibly including \[\] $\lambda\lambda6548+6583$). Although WFPC2 monochromatic emission-line images are only available for three of the objects, [@Shaw_etal06] point out that the principal, larger scale morphological features can generally be inferred from other emission lines with some confidence. We used the same classification scheme as those of @Shaw_etal01 [@Shaw_etal06] and [@Stang_etal02; @Stang_etal03], where the morphological types of relevance here are: round (R), elliptical (E), and bipolar (B). Other important structural features, such as attached shells, were noted as well.

Table \[Morph\] gives detailed information for the PNe presented here. The equatorial J2000 sky coordinates, as measured from the [*HST*]{} images, are given in columns (2) 