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Fuelling of Circumnuclear Regions: 3D Spectroscopy View.
Published online by Cambridge University Press: 01 August 2006
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.
- 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
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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
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