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The Infrared Emission Bands

Published online by Cambridge University Press:  21 February 2014

E. Peeters
E. Peeters*
Affiliation:
Department of Physics and Astronomy, University of Western Ontario, London, ON N6A 3K7, Canada email: epeeters@uwo.ca SETI Institute, 189 Bernardo Avenue, Suite 100, Mountain View, CA 94043, USA
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Abstract

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Up to 10% of the total power output of star-forming galaxies is emitted in the infrared emission features at 3.3, 6.2, 7.7, 8.6 and 11.2 μm. Here, I will review the spectral characteristics of these IR emission bands, their dependence on the local environment, the implications for the physical and chemical characteristics of the carriers, and their applicability as a diagnostic tool.

Keywords

infrared emission featuresISM: moleculesISM: lines and bands(stars:) circum-stellar matterinfrared: generalastrochemistry
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S297: The Diffuse Interstellar Bands , May 2013 , pp. 187 - 196
Copyright
Copyright © International Astronomical Union 2014 

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