is very under-abundant, which is consistent with the nebular morphology.

[*LMC–RP 1375.—*]{}The extremely low surface brightness of this object makes a definitive classification as a PN difficult, in spite of the lengthy exposure time in the WFPC2/F656N filter, but it could be a genuine PN. The morphological classification is very uncertain: the overall shape is elliptical, but it has internal structure that suggests a bipolar core (see Figure \[Neb\_3\]). The central star might be the star near the geometrical center of the nebula, but no other passbands are available for confirmation. The spectrum in Figure \[Spec\_2\] show a low level of excitation, with a low \[\]/H$\beta$ ratio, no $\lambda$4686 emission, but weak $\lambda$5876 emission.

[*LMC–RP 1550.—*]{}Despite the relatively small angular size this object is confirmed as a bipolar PN, even with the short exposure time in the WFPC2/F555W filter (see Figure \[Neb\_4\]). No central star is evident in the image. The spectrum in Figure \[Spec\_2\] indicates a moderately high level of excitation, with a high \[\]/H$\beta$ ratio and moderate $\lambda$4686 emission. The strong \[\]/H$\alpha$ ratio is consistent with the strong nebular bi-polarity [@Shaw_etal06].

Non-Detections
--------------

Of the 19 RP sources that were imaged with [*HST*]{}, extended emission was not detected 