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The presence of a Bar—Like Structure in the Central Regions of Seyfert Galaxies

Published online by Cambridge University Press:  12 April 2016

V. L. Afanasiev  and
A. I. Shapovalova
V. L. Afanasiev
Affiliation:
Special Astrophysical Observatory, Russian Academy of Sciences, Karachai-Cherkessian Republic, 357147, Russia
A. I. Shapovalova
Affiliation:
Special Astrophysical Observatory, Russian Academy of Sciences, Karachai-Cherkessian Republic, 357147, Russia

Abstract

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The central (8″ × 8″) regions of the Seyfert galaxies Mrk 744 and NGC 4151 were studied by the 3D-spectroscopy method. There is evidence that a mini-bar (0.5–2 kpc) is present in the central regions of these galaxies, which provides transportation of gas of the disk to fuel the nucleus.

Type
Posters for Part III and Part IV
Information
International Astronomical Union Colloquium , Volume 157: Barred Galaxies , 1996 , pp. 221 - 223
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

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