This photo combination shows the quasar RX J1131-1231 imaged by NASA’s Chandra X-ray Observatory and the Hubble Space Telescope. Credit: X-ray: NASA/CXC/Univ of Michigan/R.C.Reis et al; Optical: NASA/STScI
“We estimate that the X-rays are coming from a region in the disk located only about three times the radius of the event horizon — the point of no return for infalling matter,” stated Jon Miller, an an associate professor of astronomy at the University of Michigan and a co-author on the paper. “The black hole must be spinning extremely rapidly to allow a disk to survive at such a small radius.”
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Read the rest of Supermassive Black Hole’s Dizzying Spin Is Half The Speed Of Light (273 words)
© Elizabeth Howell for Universe Today, 2014. |
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Post tags: quasar, RX J1131, RX J1131-1231, supermassive black hole, University of Michigan
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