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The Far Infrared View of Star Formation in Galaxies

Published online by Cambridge University Press:  03 August 2017

Michael Rowan-Robinson
Michael Rowan-Robinson*
Affiliation:
School of Mathematical Sciences Queen Mary and Westfield College Mile End Rd, London E1 4NS

Abstract

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The contributions to the far infrared spectra of galaxies of the ‘cool’ cirrus and ‘warm’ starburst components are reviewed, together with the complications introduced by dust in the narrow-line regions of Seyferts, the destruction of very small grains, and the small percentage of galaxies which are optically thick in the optical band. The role of interactions and mergers in generating ultraluminous infrared galaxies is reviewed.

Type
VII- Infrared Emission
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 211 - 225
Copyright
Copyright © Kluwer 1991 

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