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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S275(6), p. 172-173, 2010

DOI: 10.1017/s1743921310015905

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The relation between the radio jet and the near-IR line emission in Seyfert galaxies

Journal article published in 2010 by Rogemar A. Riffel, Thaisa Storchi-Bergmann ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractWe used near-IR integral field spectroscopy, obtained with Gemini NIFS and GNIRS integral field units (IFUs), to map the ionized and molecular flux distributions and kinematics in the central few hundreds of parsecs of Seyfert galaxies. We conclude that the molecular gas emission can be considered a tracer of the feeding of the AGN, while the emission of the ionized gas a tracer of its feedback.

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