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- W2962999567 abstract "We present results based on the analysis of optical spectra of KUG 1031+398, a Narrow Line Seyfert 1 (NLS1) galaxy for which Mason et al. (1996) reported evidence for a line-emitting region intermediate (both in terms of velocity and density) between the conventional and narrow regions (BLR and NLR, respectively). From our observations and modelling of the spectra, we get a consistent decomposition of the profiles into four components: an extended H ii region with unresolved lines, two distinct Seyfert-type clouds identified with the NLR, and a relatively narrow broad line component emitting only Balmer lines but no forbidden lines. Therefore, and although we find this object to be exceptional in having line-emission from the BLR with almost the same width as the narrow lines, our interpretation of the data does not support the existence of an intermediate region (ILR)." @default.
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- W2962999567 date "1999-01-01" @default.
- W2962999567 modified "2023-10-16" @default.
- W2962999567 title "The emission-line spectrum of KUG 1031+398 and the intermediate line region ?" @default.
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