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We present an extensive, long-slit, high-resolution coverage of the complexplanetary nebula (PN), NGC 7026. We acquired ten spectra using the ManchesterEchelle Spectrometer at San Pedro Martir Observatory in Baja California,Mexico, and each shows exquisite detail, revealing the intricate structure ofthis object. Incorporating these spectra into the 3-dimensional visualizationand kinematic program, SHAPE, and using HST images of NGC 7026, we haveproduced a detailed structural and kinematic model of this PN. NGC 7026exhibits remarkable symmetry consisting of three lobe-pairs and four sets ofknots, all symmetrical about the nucleus and displaying a conical outflow.Comparing the 3-D structure of this nebula to recent, XMM-Newton X-rayobservations, we investigate the extended X-ray emission in relation to thenebular structure. We find that the X-ray emission, while confined to theclosed, northern lobes of this PN, shows an abrupt termination in the middle ofthe SE lobe, which our long slit data shows to be open. This is where theshocked, fast wind seems to be escaping the interior of the nebula and theX-ray emission rapidly cools in this region.

A Detailed Spatiokinematic Model of the Conical Outflow of the Multipolar Planetary Nebula, NGC 7026