When the matter in a globule collapses inward, it typically leads to an increase in temperature and pressure at the core. This process can trigger nuclear fusion if the conditions are right, resulting in the formation of a star. If the collapse continues beyond the fusion stage, it can lead to the formation of more compact objects like neutron stars or black holes, depending on the mass involved. The surrounding material may also be expelled, contributing to the formation of new stars and planetary systems.
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