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Observations of Infrared Emission from Galaxies

Published online by Cambridge University Press:  23 September 2016

P. F. Roche
P. F. Roche*
Affiliation:
Royal Observatory Edinburgh

Abstract

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Aspects of the infrared emission from galaxies obtained from ground-based observations are described. There are clear differences between the dust in galaxies with active nuclei and those dominated by nuclear HII regions. In particular the family of unidentified emission bands between 3 and 13 μm dominate the spectra in the latter objects, but are rarely evident in spectra of active nuclei. However results from spatial, spectral and polarization measurements show that many of the dust properties in galaxies are broadly similar to those in the Milky Way.

Type
Section IV: Dust in Galaxies
Information
Symposium - International Astronomical Union , Volume 135: Interstellar Dust , 1989 , pp. 303 - 310
Copyright
Copyright © Kluwer 1989 

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