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Infrared Line Emission by Broadly Distributed Gas

Published online by Cambridge University Press:  08 February 2017

Martin Harwit
Martin Harwit*
Affiliation:
Laboratory for Astrophysics National Air and Space Museum Smithsonian Institution Washington, DC 20560 USA

Abstract

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Diffuse infrared background radiation measurements have traditionally been carried out across broad wavelength bands, primarily because there seldom appeared to be sufficient energy available in individual spectral lines to make such observations possible. In the past few years, far-infrared searches for spectral line background radiation have become possible, and considerably greater use of these capabilities will become available in the next few years. The promise of this kind of observation is reviewed.

Type
III. Diffuse Galactic Radiation from Dust and Gas: Observations and Models
Information
Symposium - International Astronomical Union , Volume 139: The Galactic and Extragalactic Background Radiation , 1990 , pp. 149 - 155
Copyright
Copyright © Kluwer 1990 

References

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