IRAS 13224−3809 is a highly active and fluctuating Seyfert 1 galaxy in the constellation Centaurus about 1 billion light-years from Earth. The galaxy is notable due to its centrally located supermassive black hole that is closely studied by astronomers using x-ray astronomy, particularly X-ray reverberation echo mapping techniques, in an effort to better understand the inner workings, including mass and spin, of black holes.
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This article is an automated import of the Wikipedia article "IRAS 13224−3809", available at https://en.wikipedia.org/wiki/IRAS_13224%E2%88%923809 . Text is licensed under CC BY-SA 4.0.