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- W1991808051 abstract "We examine the distribution of axis ratios of a large sample of disk galaxies hosting type 2 active galactic nuclei (AGNs) selected from the Sloan Digital Sky Survey and compare it with a well-defined control sample of non-active galaxies. We find them significantly different, where the type 2 AGNs show both an excess of edge-on objects and deficit of round objects. This systematical bias cannot be explained by a nuclear obscurer oriented randomly with respect to the stellar disk. However, a nuclear obscurer coplanar with the stellar disk also does not fit the data very well. By assuming that the nuclear obscurer having an opening angle of ∼60°, we find that the observed axis ratio distribution can be nicely reproduced by a mean tilt angle of ∼30° between the nuclear obscurer and the stellar disk." @default.
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- W1991808051 date "2010-12-06" @default.
- W1991808051 modified "2023-09-23" @default.
- W1991808051 title "THE ORIENTATION OF THE NUCLEAR OBSCURER OF THE ACTIVE GALACTIC NUCLEI" @default.
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