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Gas and Stellar Kinematics in the Disk and Bar of Mrk 573

Published online by Cambridge University Press:  12 April 2016

V. L. Afanasiev ,
A. N. Burenkov ,
A. I. Shapovalova  and
V. V. Vlasyuk
V. L. Afanasiev
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, Karachai-Cherkessia, Russia, 357147
A. N. Burenkov
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, Karachai-Cherkessia, Russia, 357147
A. I. Shapovalova
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, Karachai-Cherkessia, Russia, 357147
V. V. Vlasyuk
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, Karachai-Cherkessia, Russia, 357147

Abstract

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Results of 3D-spectroscopy for the nearby Seyfert galaxy Mrk 573 obtained at the 6-m telescope with the scanning Fabry-Perot interferometer and the Multi-Pupil Field Spectrograph (MPFS) are presented. Emission lines images of the galaxy center demonstrate a complex structure of ENLR, coinciding with the radio data. An analysis of the velocity field shows that some gas structures do not lie in the plane of the galaxy. An explanation of the observed velocity field and gas distribution by radiation of a helical structure located inside an ionization cone is proposed.

Type
Posters for Part III and Part IV
Information
International Astronomical Union Colloquium , Volume 157: Barred Galaxies , 1996 , pp. 218 - 220
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Afanasiev, V.L., Dodonov, S.N., Sil’chenko, O.K., & Vlasyuk, V.V. 1990, Preprint SAO, No. 54 Google Scholar
Afanasiev, V.L. & Sil’chenko, O.K. 1991, Bull. Special Astrophys. Obs., 33, 88 Google Scholar
Ulvestad, J.S. & Wilson, A.S. 1984, ApJ, 285, 439 Google Scholar