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Infrared Emission at High Galactic Latitude

Published online by Cambridge University Press:  08 February 2017

F. Boulanger
F. Boulanger*
Affiliation:
Ecole Normale Supérieure 24 rue Lhomond 75005 Paris, France

Abstract

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Results obtained with the Infrared Astronomy Satellite (IRAS) on the IR emission at high galactic latitude are reviewed. We present evidence for the detection of galactic emission at 12, 25, 60, and 100 μm. We describe the morphology of this emission and summarize work on the correlation of IR cirrus with H I, CO, and optical emission. We discuss the contribution of the neutral atomic, ionized, and molecular gas to the total IR emission and the contribution of different components of interstellar dust to the emission seen at different wavelengths.

Information

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. 139 - 148
Copyright
Copyright © Kluwer 1990 

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