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Ages and Metallicities of Five Intermediate-Age Star Clusters Projected Towards the Small Magellanic Cloud
Published online by Cambridge University Press: 03 August 2017
Abstract
Washington CCD photometry of intermediate-age clusters in the Small Magellanic Cloud (SMC) is presented. The cluster age distribution in the SMC suggests formation epochs at 3 and 6 Gyr, respectively. Recent star formation is confined to the central body of the SMC. The chemical evolution of the SMC appears to be best represented by bursty models.
- Type
- Part 1. The Star Clusters of Local Group Galaxies
- Information
- Symposium - International Astronomical Union , Volume 207: Extragalactic Star Clusters , 2002 , pp. 196 - 198
- Copyright
- Copyright © Astronomical Society of the Pacific 2002