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Compact objects and supernova remnants provide nearby laboratories to probethe fate of stars after they die, and the way they impact, and are impacted by,their surrounding medium. The past five decades have significantly advanced ourunderstanding of these objects, and showed that they are most relevant to ourunderstanding of some of the most mysterious energetic events in the distantUniverse, including Fast Radio Bursts and Gravitational Wave sources. However,many questions remain to be answered. These include: What powers the diversityof explosive phenomena across the electromagnetic spectrum? What are the massand spin distributions of neutron stars and stellar mass black holes? How dointeracting compact binaries with white dwarfs - the electromagneticcounterparts to gravitational wave LISA sources - form and behave? Whichobjects inhabit the faint end of the X-ray luminosity function? How dorelativistic winds impact their surroundings? What do neutron star kicks revealabout fundamental physics and supernova explosions? How do supernova remnantshocks impact cosmic magnetism? This plethora of questions will be addressedwith AXIS - the Advanced X-ray Imaging Satellite - a NASA Probe Mission Conceptdesigned to be the premier high-angular resolution X-ray mission for the nextdecade. AXIS, thanks to its combined (a) unprecedented imaging resolution overits full field of view, (b) unprecedented sensitivity to faint objects due toits large effective area and low background, and (c) rapid response capability,will provide a giant leap in discovering and identifying populations of compactobjects (isolated and binaries), particularly in crowded regions such asglobular clusters and the Galactic Center, while addressing science questionsand priorities of the US Decadal Survey for Astronomy and Astrophysics(Astro2020).

From Stellar Death to Cosmic Revelations: Zooming in on Compact Objects, Relativistic Outflows and Supernova Remnants with AXIS