The Perseus–Pegasus Filament is a large-scale structure in the universe, specifically a cosmic filament, that is part of the larger cosmic web. It is a region in space where galaxies are distributed along elongated structures, often forming a network of interconnected strands, or filaments, that are separated by voids. This filament lies in the direction of the constellations Perseus and Pegasus and is known for its high density of galaxies.
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