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Star Forming Galaxies: Properties and Implications for the Extragalactic Infrared Background

Published online by Cambridge University Press:  13 May 2016

George Helou
George Helou*
Affiliation:
IPAC, Mail Code 100-22, California Institute of Technology, 1200 E. California Blvd, Pasadena, California 91125, USA

Abstract

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This paper reviews those properties of normal galaxies most relevant to the estimation of the extragalactic infrared background, in particular: (1) their infrared emission spectrum and its variation among galaxies; (2) their morphological properties, and their infrared size distribution in comparison to their apparent visible-light sizes; and (3) other properties such as the infrared-to-radio ratio and color-luminosity relations. Even a simple comparison of those properties to those of the extragalactic infrared background leads to constraints on the fluctuations in time and the secular evolutionary behavior of the infrared luminosity of galaxies.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 204: The Extragalactic Infrared Background and its Cosmological Implication , 2001 , pp. 161 - 178
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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