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On the Origin of Broad Fe Kα and H<scp>i</scp>Hα Lines in Active Galactic Nuclei
We examine the properties of the Fe emission lines that arise near 6.4 keV in the ASCA spectra of AGNs. Our emphasis is on the Seyfert 1 galaxies where broad and apparently complex Fe Kα emission is observed. We consider various origins for the line but focus on the pros …