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- W2014071871 abstract "We present theoretical Fe I-III emission-line strengths for physical conditions typical of Active Galactic Nuclei with Broad-Line Regions. We can satisfactorily reproduce the empirical UV Fe II-III emission-line template of Vestergaard & Wilkes (2001) for the prototypical narrow-line Seyfert 1 galaxy I Zw 1, although a number of detailed discrepancies remain.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html" @default.
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- W2014071871 date "2004-03-01" @default.
- W2014071871 modified "2023-09-26" @default.
- W2014071871 title "Predicted Fe I-III fluxes for AGNs with BLRs" @default.
- W2014071871 doi "https://doi.org/10.1017/s1743921304002625" @default.
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