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Low-redshift Galaxies in the Infrared and Submillimetre

Barnard, V. E. and Blain, A. W. (2002) Low-redshift Galaxies in the Infrared and Submillimetre. Astrophysics and Space Science, 281 (1-2). pp. 525-526. ISSN 0004-640X. doi:10.1023/a:1019585801494. https://resolver.caltech.edu/CaltechAUTHORS:20191127-134853623

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Abstract

In recent years the evolution of dust-enshrouded galaxies has become an important issue in cosmology. We present the results of a study linking the high- and low-redshift populations of such galaxies. Previously, a simple hierarchical clustering model was found to be successful in describing the high-redshift populations of dusty galaxies. This study showed that strong evolution could not be avoided in order to satisfy all the high-redshift infrared and submillimetre constraints. We now apply the same model to the low-redshift data available, and find that the strong evolution inferred is compatible with the count and redshift data we have from IRAS, ISO and SCUBA.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1023/a:1019585801494DOIArticle
https://rdcu.be/bXMivPublisherFree ReadCube access
ORCID:
AuthorORCID
Blain, A. W.0000-0001-7489-5167
Additional Information:© 2002 Kluwer Academic Publishers.
Subject Keywords:Galaxies: evolution; galaxies: interactions; infrared: galaxies
Issue or Number:1-2
DOI:10.1023/a:1019585801494
Record Number:CaltechAUTHORS:20191127-134853623
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191127-134853623
Official Citation:Barnard, V. & Blain, A. Astrophysics and Space Science (2002) 281: 525. https://doi.org/10.1023/A:1019585801494
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:100113
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:28 Nov 2019 01:57
Last Modified:16 Nov 2021 17:51

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