The flux ratio of the [O III] 5007, 4959 lines in AGN: comparison with theoretical calculations
M. S. Dimitrijević(Centre National de la Recherche Scientifique), D. Ilić(Universität Hamburg), Luka Č. Popović(Chinese Academy of Sciences), Jelena Kovačević(University of Belgrade), M. Dačić(Astronomical Observatory)
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