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 | |||||||||
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| 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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