What are the denser regions within a Giant Molecular Cloud called that act as direct precursors to individual stars?
Cores
Star formation does not typically begin uniformly across an entire Giant Molecular Cloud (GMC); rather, it initiates in localized areas where gravitational forces have managed to create sufficient density enhancements. These localized, self-gravitating regions are specifically termed 'cores.' These cores represent the stage where density is high enough—often orders of magnitude greater than the surrounding cloud—that the Jeans Mass criterion for gravitational collapse is met or exceeded. Finding these internal clumps within the larger GMC complex provides the observational proof that gravitational fragmentation is successfully taking place, marking these cores as the immediate, direct precursors that will eventually evolve into a single star or a small star system.
