New stars are typically born from molecular clouds, also known as nebulae. Within these dense regions of gas and dust, gravitational forces can cause clumps of material to collapse, leading to the formation of new stars. Multiple stars can form from a single nebula, often resulting in star clusters where several stars are born simultaneously from the same material. Examples of well-known star-forming nebulae include the Orion Nebula and the Eagle Nebula.
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