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Obscured Activity: AGN, Quasars, Starbursts and ULIGs Observed by the Infrared Space Observatory

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Abstract

Some of the most ‘active’ galaxies in the Universe are obscured by large quantities of dust and emit a substantial fraction of their bolometric luminosity in the infrared. Observations of these infrared luminous galaxies with the Infrared Space Observatory (ISO) have provided a relatively unabsorbed view to the sources fuelling this active emission. The improved sensitivity, spatial resolution and spectroscopic capability of ISO over its predecessor Infrared Astronomical Satellite (IRAS) of enabled significant advances in the understanding of the infrared properties of active galaxies. ISO surveyed a wide range of active galaxies which, in the context of this review, includes those powered by intense bursts of star formation as well as those containing a dominant active galactic nucleus (AGN). Mid-infrared imaging resolved for the first time the dust enshrouded nuclei in many nearby galaxies, while a new era in infrared spectroscopy was opened by probing a wealth of atomic, ionic and molecular lines as well as broad band features in the mid- and farinfrared. This was particularly useful, since it resulted in the understanding of the power production, excitation and fuelling mechanisms in the nuclei of active galaxies including the intriguing but so far elusive ultraluminous infrared galaxies. Detailed studies of various classes of AGN and quasars greatly improved our understanding of the unification scenario. Far-infrared imaging and photometry revealed the presence of a new very cold dust component in galaxies and furthered our knowledge of the far-infrared properties of faint starbursts, ULIGs and quasars. We summarise almost nine years of key results based on ISO data spanning the full range of luminosity and type of active galaxies.

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Author notes

  1. Vassilis Charmandaris (Chercheur Associé)

    Present address: Department of Physics, University of Crete, GR-71003, Heraklion, Greece

Authors and Affiliations

  1. Max-Planck Institut für extraterrestrische Physik, Postfach 1312, D-85741, Garching, Germany

    Aprajita Verma & Dieter Lutz

  2. Department of Astronomy, Cornell University, 106 Space Sciences Building, Ithaca, NY, 14853, USA

    Vassilis Charmandaris (Chercheur Associé)

  3. Observatoire de Paris, F-75014, Paris, France

    Vassilis Charmandaris (Chercheur Associé)

  4. Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117, Heidelberg, Germany

    Ulrich Klaas

  5. Astronomisches Institut, Ruhr-Universität, Universitätsstr 150, D-44780, Bochum, Germany

    Martin Haas

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  1. European Southern Observatory, Garching, Munich, Germany

    Catherine Cesarsky

  2. European Space Agency, Madrid, Spain

    Alberto Salama

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Verma, A., Charmandaris, V., Klaas, U., Lutz, D., Haas, M. (2005). Obscured Activity: AGN, Quasars, Starbursts and ULIGs Observed by the Infrared Space Observatory. In: Cesarsky, C., Salama, A. (eds) ISO Science Legacy. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3844-5_15

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