Anti-correlation between Fe II equivalent width and FWHM underlies the quasar main sequence, driven mainly by strengthening of inconsistent lines and ILR components.
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Unravelling the complex structure of the Fe II emission region in Type 1 active galactic nuclei
Anti-correlation between Fe II equivalent width and FWHM underlies the quasar main sequence, driven mainly by strengthening of inconsistent lines and ILR components.
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