A Multi-Wavelength Investigation of Seyfert 1.8 and 1.9 Galaxies
We focus on determining the underlying physical cause of a Seyfert galaxy's appearance as type a 1.8 or 1.9. Are these "intermediate" Seyfert types typical Seyfert 1 nuclei reddened by central dusty tori or by nuclear dust lanes/spirals in the narrow-line region? Or, are they similar...
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| Format: | Others |
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Digital Archive @ GSU
2009
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| Online Access: | http://digitalarchive.gsu.edu/phy_astr_diss/35 http://digitalarchive.gsu.edu/cgi/viewcontent.cgi?article=1034&context=phy_astr_diss |