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- W2016030167 abstract "luminosities yet observed. We compare UB3 to known Fe II strong objects and also consider possible correlations between Fe II strength and other observables. We confirm a previous suggestion that Fe II strong objects are among the most FIR luminous AGN. UB3 also confirms the tendency for Fe II strong objects to have relatively narow Hβ and weak [O III]λ5007 A emission. We consider the possibility that UB3 may have unusually weak or absent UV Fe II features. If confirmed, this would suggest that the optical Fe II features are in a very dense region in which UV lines are suppressed by radiative transfer effects." @default.
- W2016030167 created "2016-06-24" @default.
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- W2016030167 date "1990-11-01" @default.
- W2016030167 modified "2023-09-26" @default.
- W2016030167 title "N2841-UB3 - A QSO with unusually strong optical Fe II emission" @default.
- W2016030167 doi "https://doi.org/10.1086/132762" @default.
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