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Dense molecular gas disks drive the growth of supermassive black holes
Dense molecular gas disks drive the growth of supermassive black holes: Are supernova explosions the key?
Astronomers have revealed that dense molecular gas disks a few hundred light years in scale located at the centers of galaxies supply gas to supermassive black holes situated within them. This finding provides important insights on the growth of supermassive black holes over cosmic time.
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