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- W2000260310 abstract "(~10 kpc; ~135), diffuse ionized medium (DIM) recently detected in the nearby, luminous Seyfert galaxy NGC 1068. The DIM phase was recognized from spectrophotometric Hα and [N II] λλ6548,6584 line emission maps obtained with the Hawaii Imaging Fabry-Perot Interferometer (HIFI). We demonstrate that the Hot equivalent-width distribution, when combined with the [N II] λ6584/Hα line ratio distribution, permits a clean separation of the DIM from the adjacent H II region population. We summarize the main reasons that lead us to believe the DIM is photoexcited predominantly by scattered light from the active nucleus rather than the extended stellar population." @default.
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- W2000260310 date "1991-08-01" @default.
- W2000260310 modified "2023-09-26" @default.
- W2000260310 title "Diffuse ionized medium in NGC 1068" @default.
- W2000260310 doi "https://doi.org/10.1086/132905" @default.
- W2000260310 hasPublicationYear "1991" @default.
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