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Infrared Properties of Nearby Interacting Galaxies: from Spirals to ULIRGs

Published online by Cambridge University Press:  01 August 2006

Vassilis Charmandaris
Vassilis Charmandaris*
Affiliation:
Department of Physics, University of Crete, P.O. Box 2208, Heraklion, 71003, Greece email: vassilis@physics.uoc.gr
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Abstract

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I present a brief review of some of the mid-infrared properties of interacting galaxies as these were revealed using observations from the Infrared Space Observatory and Spitzer Space Telescope over the last decade. The variation of the infrared spectral energy distribution in interacting galaxies can be used as an extinction free tracer not only of the location of the star formation activity but also of the physical mechanism dominating their energy production.‡.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 180 - 183
Copyright
Copyright © International Astronomical Union 2007

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