低光度塞弗特2星系和活動星系核統(tǒng)一模型.pdf

1、Using Shu et al., 2007's "Investigating The Nuclear Obscuration in Two Typesof Seyfert 2 Galaxies' (Shu et al., 2007)" as a prototype, we demonstrated that highsignal-to-noise ratio and better spatially resolved data can

2、 account for some of the ob-servations that are inconsistent with the Unification models of Active Galactic Nuclei.New data for the relatively Iow luminous seyfert 2 sources((seyfert 2 with luminos-ity < 1041e,rg/s), whi

3、ch wouldn't be incorporated in the conclusions of Shu et al.,2007, are sought for and analyzed, to examine whether doing so would lead to the in-clusion all of all of Shu et al.'s sample into their conclusions. We accomp

4、lished thattask successfully and then embarked on the slippery slope of questioning some high-ly cherished concepts upon which current understandings of Active Galactic Nucleiare anchored and in doing so provided persona