Hubble Space Telescope images of NGC 6543 taken in 1994.7 through a variety of narrowband filters yield a very detailed structure in emission lines of low and moderate ionization. On the whole, the core of NGC 6543 is optically thin to ionizing radiation. As expected, the general ionization state of the nebula decreases with radius; however, some of the fluctuations are unexpectedly large in scale and impressive in their complex geometries. Other sinewy or arclike features near the edge of the core, known as the "caps," "ansae," and "jets," are extremely low in ionization. The images show that they are made up of closely packed complexes of very dense knots whose recombination times are 10 yr. Furthermore, we find thin and perfectly radial features that we interpret as ionization shadows behind many of the dense knots. Image ratios show no detectable microscopic or macroscopic changes in electron temperature Te seen in the [O III] lines even though the densities probably range between 103 and 105 cm-3 in various regions. Finally, no internal variations of extinction or the He+/H+ ratios are found within the core.
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