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String of young clusters linking the Magellanic Clouds
Published online by Cambridge University Press: 19 July 2016
Abstract
We present deep CCD photometry of three associations lying between the Magellanic Clouds and sitting on the HI ridge. ZAMS fittings show that these clusters are located at the distance of the Clouds. Furthermore, a slight distance gradient is observed. Main sequences matched to isochrones reveal that these aggregates are very young, no more than 108 years old. An age difference from east to west is also suggested.
- Type
- The LMC-SMC-Galaxy System
- Information
- Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 478 - 479
- Copyright
- Copyright © Kluwer 1991
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