Title: An ultra-luminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30 Author: Xue-Bing Wu, Feige Wang, Xiaohui Fan, Weimin Yi, Wenwen Zuo, Fuyan Bian, Linhua Jiang, Ian D. McGreer, Ran Wang, Jinyi Yang, Qian Yang, David Thompson, Yuri Beletsky
So far, roughly 40 quasars with redshifts greater than z=6 have been discovered. Each quasar contains a black hole with a mass of one billion solar masses ( 109 solar masses). The existence of such black holes when the Universe was less than 1 billion years old presents substantial challenges to theories of the formation and growth of black holes and the coevolution of black holes and galaxies. Here we report the discovery of an ultra-luminous quasar, SDSS J010013.02+280225.8, at redshift z=6.30. It has an optical and near-infrared luminosity a few times greater than those of previously known z>6 quasars. On the basis of the deep absorption trough on the blue side of the Ly alpha emission line in the spectrum, we estimate the proper size of the ionised proximity zone associated with the quasar to be 26 million light years, larger than found with other z>6.1 quasars with lower luminosities. We estimate (on the basis of a near-infrared spectrum) that the black hole has a mass of ~1.2 x 1010 solar masses, which is consistent with the 1.3 x 1010 solar masses derived by assuming an Eddington-limited accretion rate.
Ancient black hole had an inexplicable growth spurt
Astronomers have discovered a black hole with a mass 12 billion times that of the sun. It seems to have reached that size when the universe was less than a billion years old, which creates a puzzle. Current models suggest that it could not have grown so big so soon after the big bang. Read more