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Dusty Tori of Seyfert Nuclei Probed by the Water Vapor Maser Emission: How Large Are the Dusty Tori?
1998
Astrophysical Journal
Geometrical and physical properties of dusty tori of Seyfert nuclei probed by the water vapor maser emission at 22 GHz are discussed. We assume that the dusty torus has a simple cylindrical form and the maser emission can be detected only when we observe the torus from almost edge-on views. The observed low frequency of occurrence of the water vapor maser emission (less than 10 percent) suggests that the torus is a vertically thin cylinder whose outer radius between a few pc and ~ 10 pc.
doi:10.1086/311435
fatcat:nhsldlafyfbrvdhf6ixpm6bv3u