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IRAS 13224-3809 is a highly active and flu … 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., including mass and spin, of black holes.
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IRAS 13224-3809
, 2MASX J13251937-3824524; 2MASS J13251937-3824526; GSC 07787-00931; IRAS F13224-3809; 1RXS J132519.4-382445; WISE J132519.39-382452.5; Gaia DR2 6162481890199388928
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rdfs:comment |
IRAS 13224-3809 is a highly active and flu … 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., including mass and spin, of black holes.
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rdfs:label |
IRAS 13224-3809
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