Poster abstract details

We discuss the three dimensional morphology, ionization structure, and kinematics of NGC 2392, the "Eskimo," based on new and archival HST imagery and new long-slit echelle and integral field spectroscopy. High spatial resolution 2D ionization maps of the nebula were made from the HST WFPC2 imagery and compared with maps of the emission-line structure in weaker diagnostic lines from the VIRUS-P IFS observations obtained at McDonald Observatory. Then high velocity resolution long-slit spectroscopy with the KPNO 4m echelle spectroscopy was used to map the kinematics and evaluate the 3D ionization structure of the nebula in several important ions, including C++ for the first time.