Cohen, J. G. and Rich, R. M. and Persson, S. E. (1984) IUE observations of the clusters of the Magellanic Clouds. Astrophysical Journal, 285 . pp. 595-600. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20190531-091632986
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Abstract
IUE observations of 17 clusters in the Large Magellanic Cloud are presented. The derived ultraviolet colors become progressively redder as the cluster's classification in the scheme of Searle, Wilkinson, and Bagnuolo increases. With the aid of theoretical models of the integrated light of coeval clusters of varying ages, it is shown that the SWB classification is one of increasing age accompanied by decreasing metallicity toward later SWB classes. The behavior of the UV absorption line features in the integrated light of the LMC clusters supports the contention.
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| Additional Information: | © American Astronomical Society • Provided by the NASA Astrophysics Data System. Received 1984 January 25; accepted 1984 May 2. We are grateful to NASA (grant NAG 5-63) for financial support and to the IUE Observatory staff for helpful advice. | |||||||||
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| Subject Keywords: | clusters: globular - galaxies: Magellanic Clouds - ultraviolet: spectra | |||||||||
| Record Number: | CaltechAUTHORS:20190531-091632986 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20190531-091632986 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 95992 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | George Porter | |||||||||
| Deposited On: | 03 Jun 2019 21:38 | |||||||||
| Last Modified: | 03 Oct 2019 21:18 |
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