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Infrared to Millimeter Spectroscopy and Imaging of Active Galactic Nuclei

Published online by Cambridge University Press:  12 April 2016

R. Genzel ,
D. Lutz ,
E. Sturm ,
L. Tacconi ,
N. Thatte  and
A. Sternberg
R. Genzel
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik, Postfach 1603, D-85740 Garching, Germany
D. Lutz
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik, Postfach 1603, D-85740 Garching, Germany
E. Sturm
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik, Postfach 1603, D-85740 Garching, Germany
L. Tacconi
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik, Postfach 1603, D-85740 Garching, Germany
N. Thatte
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik, Postfach 1603, D-85740 Garching, Germany
A. Sternberg
Affiliation:
School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978, Israel

Abstract

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Observations in the 1 µm to 1 cm wavelength band give important information on the physical processes occurring in and immediately around active galactic nuclei. Concentrating on recent results on ionic, atomic, and molecular emission lines, we discuss as examples the first ISO results on the nature of ultra-luminous infrared galaxies, and near-infrared and millimeter measurements of the central 100 parsecs of the Seyfert 2 galaxy NGC 1068.

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. 312 - 324
Copyright
Copyright © Astronomical Society of the Pacific 1997

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