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Testing Intermediate-age Stellar Evolution with Magellanic Cloud Clusters
Published online by Cambridge University Press: 03 August 2017
Abstract
We present new deep VLT color-magnitude diagrams of three intermediate-age populous star clusters in the LMC. These data will be used independently by the Padova and Yale stellar evolution Groups to address issues relevant to the evolution of intermediate-mass stars: mainly the extent of the core convective overshoot, as well as other poorly determined parameters, such as mass loss during stellar evolution, internal rotation, and He content.
- Type
- Part 4. Star Cluster Formation and Evolution: Theory and Observation
- Information
- Symposium - International Astronomical Union , Volume 207: Extragalactic Star Clusters , 2002 , pp. 713 - 715
- Copyright
- Copyright © Astronomical Society of the Pacific 2002