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Integral Field Spectrography of Active Galaxies with TIGER

Published online by Cambridge University Press:  12 April 2016

P. Ferruit ,
E. Pécontal ,
G. Adam  and
R. Bacon
P. Ferruit
Affiliation:
CRAL Observatoire de Lyon, UMR CNRS 5574, F–69561 Saint-Genis-Laval Cedex, France
E. Pécontal
Affiliation:
CRAL Observatoire de Lyon, UMR CNRS 5574, F–69561 Saint-Genis-Laval Cedex, France
G. Adam
Affiliation:
CRAL Observatoire de Lyon, UMR CNRS 5574, F–69561 Saint-Genis-Laval Cedex, France
R. Bacon
Affiliation:
CRAL Observatoire de Lyon, UMR CNRS 5574, F–69561 Saint-Genis-Laval Cedex, France

Abstract

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The TIGER integral field spectrograph has been used to study nearby and distant active galaxies. We first present new TIGER observations of the Seyfert galaxy NGC 1275. In this very complex object, TIGER allows us to disentangle the contributions of the numerous components. We present the first very promising results on NGC 5252 obtained with the 3-D data-cube deconvolution techniques developed by our team in Lyon.

Type
VI. The Narrow-Line Regions and Beyond
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 343 - 346
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

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