Reflection from the strong gravity regime in a lensed quasar at redshift z = 0.658

R. C. Reis (), M. T. Reynolds, J. M. Miller and D. J. Walton
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R. C. Reis: University of Michigan
M. T. Reynolds: University of Michigan
J. M. Miller: University of Michigan
D. J. Walton: Cahill Center for Astronomy and Astrophysics, California Institute of Technology

Nature, 2014, vol. 507, issue 7491, 207-209

Abstract: Observations of a gravitationally lensed quasar at redshift 0.658 imply a high spin parameter, which indicates that this supermassive black hole grew by coherent accretion rather than in a chaotic manner.

Date: 2014
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DOI: 10.1038/nature13031

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