Stellar feedback is the process where stars influence their environment through radiation, winds, and supernovae.Stellar feedback is the collective influence that stars exert on their surrounding interstellar medium through radiation, stellar winds, and supernova explosions. This process is a fundamental driver of galaxy evolution, regulating star formation rates, shaping the structure of the interstellar medium, and enriching it with heavy elements. Without feedback, galaxies would convert all their gas into stars much faster than observed, so feedback is the key self-regulating mechanism that keeps star formation inefficient.
The concept was recognized in the mid-20th century, with early work by Lyman Spitzer and others on supernova remnants. The term 'stellar feedback' became widely used in the 1990s as numerical simulations of galaxy formation required a prescription for this process to match observations.
Massive stars emit intense ultraviolet radiation that ionizes and heats surrounding gas, creating expanding bubbles. Their fast stellar winds push material outward, and when they explode as supernovae, they inject enormous amounts of energy and momentum into the interstellar medium, compressing gas and triggering or suppressing star formation in different regions. The combined effect of these processes can drive galactic-scale outflows, expelling gas from the galaxy entirely.
It is essential for accurate simulations of galaxy formation and evolution, and for interpreting observations of star-forming regions and galactic winds in the context of cosmology.
The Lyman-alpha radiation from young stars can be so intense that it literally pushes gas clouds apart, a process that may have played a role in ending the 'cosmic dark ages' and reionizing the universe.

