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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



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ID: 276703.0, MPI für Astronomie / Publikationen_mpia
Obscured activity: AGN, quasars, starbursts and ULIGs observed by the Infrared Space Observatory
Authors:Verma, Aprajita; Charmandaris, Vassilis; Klaas, Ulrich; Lutz, Dieter; Haas, Martin
Language:English
Date of Publication (YYYY-MM-DD):2005
Title of Journal:Space Science Reviews
Journal Abbrev.:Space Science Reviews
Volume:119
Start Page:355
End Page:407
Review Status:not specified
Audience:Not Specified
Abstract / Description: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 far-infrared. 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.
Free Keywords:galaxies: active; galaxies: starburst; galaxies: Seyfert; galaxies: quasars; infrared: galaxies
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/cgi-bin/nph- bib_query?b... [ID No:1]
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