  Stellar and black hole feedback heat and disperse surrounding cold gas
clouds, launching gas flows off circumnuclear and galactic disks and producing
a dynamic interstellar medium. On large scales bordering the cosmic web,
feedback drives enriched gas out of galaxies and groups, seeding the
intergalactic medium with heavy elements. In this way, feedback shapes galaxy
evolution by shutting down star formation and ultimately curtailing the growth
of structure after the peak at redshift 2-3. To understand the complex
interplay between gravity and feedback, we must resolve both the key physics
within galaxies and map the impact of these processes over large scales, out
into the cosmic web. The Advanced X-ray Imaging Satellite (AXIS) is a proposed
X-ray probe mission for the 2030s with arcsecond spatial resolution, large
effective area, and low background. AXIS will untangle the interactions of
winds, radiation, jets, and supernovae with the surrounding ISM across the wide
range of mass scales and large volumes driving galaxy evolution and trace the
establishment of feedback back to the main event at cosmic noon.
