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Young Populous Clusters in the Magellanic Clouds – Implications for Stellar Evolutionary Models
Published online by Cambridge University Press: 25 May 2016
Abstract
We present new UV, visual and Hα photometry obtained with the WFPC2 of NGC 330, NGC 1818, NGC 2004 and NGC 2100, four young populous clusters in the MCs. We present observational evidence for a degree of convective core overshoot in excess of that currently applied in standard models.
- Type
- Part 6. Stellar Clusters
- Information
- Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 436 - 437
- Copyright
- Copyright © Astronomical Society of the Pacific 1999
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