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Fuelling of Circumnuclear Regions: 3D Spectroscopy View.

Published online by Cambridge University Press:  01 August 2006

A. V. Moiseev  and
A. A. Smirnova
A. V. Moiseev
Affiliation:
Special Astrophysical Observatory, Russian Academy of Sciences, 369167Russia email: moisav@sao.ru
A. A. Smirnova
Affiliation:
Special Astrophysical Observatory, Russian Academy of Sciences, 369167Russia email: moisav@sao.ru
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Abstract

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We review the results recently obtained by means of panoramic (3D) spectroscopy on the 6-m telescope BTA (SAO RAS). This research is devoted to observational evidences of gas inflow into the centers of galaxies, which must ensure the fueling of an active nucleus. 3D spectroscopy allows us to trace the behavior of gas and stars in the one-kiloparsec size vicinity of an AGN and also far from the center.

Keywords

galaxies: Seyfertgalaxies: jetsgalaxies: kinematics and dynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 125
Copyright
Copyright © International Astronomical Union 2007

References

Amram, P., Plana, H., Mendes de Oliveira, C., Balkowski, C., & Boulesteix, J., 2003, A&A, 402, 865.Google Scholar
Smirnova, A.A., Moiseev, A.V., & Afanasiev, V.L., 2006a, Astronomy Letters, 32, 520, astro-ph/0607163.CrossRefGoogle Scholar
Smirnova, A.A., Gavrilović, N., Moiseev, A.V., & PopovićL., Č. L., Č., 2006b, MNRAS, submitted.Google Scholar