Supernova Remnants and Pulsar Wind Nebulae in the Chandra Era

X-ray observatories are advancing our understanding of a wide range of astrophysical processes, and profoundly so in the field of supernova remnants. The Chandra X-ray Observatory's superior spatial and spectral resolution, for example, are probing the structure and evolution of supernova remnant ejecta, diffusive shock acceleration processes, and interactions between supernova remnants and pulsar wind nebulae down to the sub-arcsecond level. This conference highlights both observational and theoretical studies of SNR, emphasizing recent X-ray observations of Galactic SNR. All aspects of SNR research will be explored including shock acceleration, electron/ion temperature equilibration, pulsar wind nebulae, connections between SNR ejecta and SN processes, and SNR interactions with the circumstellar and interstellar medium. The goals are to discuss outstanding problems in SNR research, and the most direct path forward in coming years.