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A nebula may begin to shrink due to gravitational forces overcoming the internal pressure that was previously keeping it expanded. As the gas and dust within the nebula cools and condenses, gravity pulls the material together, leading to a denser region that can eventually form stars. Additionally, external influences such as shock waves from nearby supernovae can compress the nebula, accelerating the process of contraction. This shrinking can initiate the formation of new stellar objects within the nebula.

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