Star formation
Star formation refers to the physical processes by which dense regions within molecular clouds collapse to form stars. It involves gravitational contraction, radiative processes, and interactions with surrounding matter.
Star formation is discussed in astrophysics, galactic astronomy, and plasma physics.
Status
Star formation is studied through observation of molecular clouds, protostellar objects, and young stellar populations. Models address the roles of turbulence, magnetic fields, and feedback processes, and remain under active development.