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- W4245246836 abstract "Because of the metastability of the 2 3 S level of He I, a variety of effects can change the line strengths from pure recombination values in Seyfert galaxies (see Feldman and MacAlpine 1978). This occurs because the population which builds up in the 2 3 S level can be collisionally excited to the 2 3 P level, enhancing λ10830. The expected ratios of λ10830/λ5876 can be altered by internal or external reddening and vary with temperature, density and optical depth." @default.
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- W4245246836 date "1989-01-01" @default.
- W4245246836 modified "2023-10-18" @default.
- W4245246836 title "Helium I λ10830 Observations of Seyfert 2 Galaxies" @default.
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- W4245246836 doi "https://doi.org/10.1017/s0074180900140604" @default.
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