September 15, 2016

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Supermassive black holes, millions to billions of times the mass of our Sun, are found at the centers of galaxies. Many are hidden within a thick doughnut-shape ring of dust and gas known as a torus. Previous observations suggested these cloaking structures are formed from native material found near the galaxy's center. New data from NSF-funded Atacama Large Millimeter/submillimeter Array reveal that one such black hole is actually the source of its own dusty torus of dust and gas.Full Story

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National Radio Astronomy Observatory

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