between the inner bright ring and the outer halo, and at the same radial distance as the ansae.

The spectra are shown in Figure 7. The bright core is dominated by stellar continuum emission. The other positions show strong line emission. The spectrum labeled SW Lobe was taken on the inner bright ring directly SW of the central star. The SW Halo position was taken in the halo midway between the bright ring and the outer edge of the PN. The lobe and halo emission is similar, except for relatively brighter lines of at 1.7002  in the lobe. There is also some continuum emission at the short wavelength end of the nebular positions, which is probably scattered light from the central star.

### NGC 7009

NGC 7009 (the “Saturn” nebula) is an elliptical with an interesting twisted symmetry in its shell and in the various filaments and knots of emission. Balick et al. (1998) recently published HST images that show the “microstructures” in this PN. The images show that the inner knots are actually groups of FLIERs, and jets in \[\] are seen that terminate at the tips of the nebula.

Two positions were sampled, one in the halo region 