The radiative energy put back to the environment through an astrophysical
process. For example, in the process of → star formation → accretion disks form around → protostars.
The material in the disk spirals
inward and on to the protostar, provided that there is an efficient
mechanism to redistribute → angular momentum
outward in the disk. During this process
→ gravitational energy is transformed into
radiation due to → viscous dissipation
in the disk and at the → accretion shock
around the protostar. This radiation heats the region around the protostar and
may → suppress
subsequent → fragmentation
and further star formation.
Thus, radiative feedback plays a critical role in regulating the stellar
→ initial mass function.