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Possible evidence for a massive black hole in a quasar with double redshift systems
Authors:Yong-Zhen Liu  Zu-Gan Deng  You-Yuan Zhou  Jie-Hao Huang
Institution:(1) Department of Physics, Graduate School, University of Science and Technology of China, Beijing, China;(2) Center of Astrophysics, University of Science and Technology of China, Hefei, China;(3) Department of Astronomy, Nanjing University, Nanjing, China
Abstract:With the aid of a simple black hole model of quasars we have found that the majority of the distinguishable emission lines in the spectrum of the quasar 1604+179 can be assigned to two redshift systems,z r =3.712 andz b =2.701. The appearance of double emission redshifts means that this quasar might be a massive black hole (of mass 108 M bullleMle1011 M bull) with a ring-like emission line region (of radius 1 light-day ler 0le1 light-year) in its accretion disk.
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