Helical structures in Seyfert galaxies

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dc.creatorMoiseev, A. V.
dc.creatorAfanasiev, V. L.
dc.creatorDodonov, S. N.
dc.creatorMustsevoi, V. V.
dc.creatorKhrapov, S. S.
dc.date2001-11-12
dc.date.accessioned2026-07-07T02:01:19Z
dc.date.available2026-07-07T02:01:19Z
dc.descriptionThe Seyfert galaxies with Z-shaped emission filaments in the Narrow Line Region (NLR) are considered. We assume that observable Z-shaped structures and velocity pattern of NLR may be explained as tridimensional helical waves in the ionization cone.
dc.descriptionTo appear in IAU Colloq. 184, AGN Surveys, ed. R. F. Green, E. Ye. Khachikian, & D. B. Sanders (San Francisco: ASP), in press. 2 pages, 1 EPS figure
dc.identifierhttps://arxiv.org/abs/astro-ph/0111217
dc.identifierhttp://arxiv.org/abs/astro-ph/0111217
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3703
dc.subjectAstrophysics
dc.titleHelical structures in Seyfert galaxies
dc.typetext

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