geometric center of the nebula, and is tentatively identified through its $B-V$ color. The spectrum in Figure \[Spec\_1\] indicates a fairly high excitation, with a large \[\]/H$\beta$ ratio and relatively strong $\lambda$4686 emission.

[*LMC–RP 764.—*]{}This object is clearly a bipolar PN and is similar in appearance to the Dumbbell nebula (see Figure \[Neb\_2\]). The identification of the central star is puzzling: based on the F330W image, a star at the northwest edge of the nebula is by far the bluest in the image, and is the best candidate. The spectrum in Figure \[Spec\_2\] indicates a moderate level of excitation, with a moderate \[\]/H$\beta$ ratio and finite $\lambda$4686 emission. The very strong \[\]/H$\alpha$ ratio (more than 4:1) is consistent with the strong nebular bi-polarity [@Shaw_etal06].

[*LMC–RP 885.—*]{}This object is confirmed as a round, faint PN. It has a main shell of $\sim0.27$ pc in diameter, and has an attached shell that is twice as large but fainter by a factor of at least 3 (see Figure \[Neb\_3\]). The central star is relatively bright. The spectrum in Figure \[Spec\_2\] indicates a very high excitation, with a large \[\]/H$\beta$ ratio and very strong $\lambda$4686 emission. The absence of \[\] emission suggests that N 