slit was centered on the object, and includes the star as well as the nebular emission that is typical of this class of PN.

### NGC 6803

This compact elliptical PN has a uniformly bright disk with no apparent structure in the optical, and is surrounded by a fainter halo about twice the size of the bright shell (Schwarz et al. 1992). In the KSPEC imaging channel, however, the PN was seen to be double-lobed, with the lobes on the minor axis of the bright elliptical region. Spectra were obtained at two positions, one centered on the E lobe, and the other position 5 arcseconds NW in the halo region. The lobe spectrum shows bright and lines, with a stellar continuum contribution out to about 1.5 . There is also unidentified line emission at 2.286 . The halo spectrum is quite different, with weak  and continuum emission, and is probably reflected star and nebular emission.

### NGC 6826

This elliptical PN is morphologically similar to NGC 3242, with a bright elliptical inner ionized ring, ansae along the major axis, and a fainter halo that envelopes the system (Balick 1987). The I-band image in Paper I shows evidence for a shell 