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Partly obscured accretion disc model to explain shifted broad Balmer emission lines of active galactic nuclei
Authors:Xue-Guang Zhang  Deborah Dultzin  Ting-Gui Wang  Guinevere Kauffmann
Institution:Max-Plank-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85748 Garching, Germany;Instituto de Astronomia, Universidad Nacional Autonoma de Mexico, Apdo Postal 70-264, Mexico DF 04510, Mexico;Center for Astrophysics, Department of Astronomy and Applied Physics, University of Science and Technology of China, Hefei, Anhui, China
Abstract:
Keywords:galaxies: active  galaxies: nuclei  quasars: emission lines
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