IC 348 is a young open cluster located in the constellation Perseus. It is part of the Perseus molecular cloud and is approximately 3 million years old. The cluster contains a significant number of young stars, some of which are still in the process of forming. IC 348 is notable for its high-density region of young stellar objects, and it has been studied extensively in various wavelengths, including infrared and X-ray, to learn about star formation processes.
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