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Helical Structures in Seyfert Galaxies
Published online by Cambridge University Press: 12 April 2016
Abstract
Seyfert galaxies with Z-shaped emission filaments in the Narrow Line Region (NLR) are considered. We assume that observable Z-shaped structures and the velocity pattern of the NLR may be explained as tri-dimensional helical waves in the ionization cone.
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- Part 5. AGN Phenomena
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- Copyright © Astronomical Society of the Pacific 2002
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