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Supernova remnants serve as nearby laboratories relevant to many areas inAstrophysics, from stellar and galaxy evolution to extreme astrophysics and theformation of the heavy elements in the Universe. The Chandra X-ray mission hasenabled a giant leap forward in studying both SNRs and their compact stellarremnants on sub-arcsecond scale. However, such high-resolution imaging studieshave been mostly limited to the nearby and/or relatively bright objects. Thereis no question that we are missing a large population, especially in externalgalaxies. Within our own Galaxy, we are presented with new fundamentalquestions related to neutron stars' diversity, kicks, relativistic winds andthe way these objects interact with, and impact, their host environments. Inthis white paper, we highlight some of the breakthroughs to be achieved withfuture X-ray missions (such as the proposed AXIS probe) equipped withsub-arcsecond imaging resolution and an order of magnitude improvement insensitivity.

High-Resolution X-ray Imaging Studies of Neutron Stars, Pulsar Wind Nebulae and Supernova Remnants