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| Paper: |
Young Populous Clusters in the Magellanic Clouds. |
| Volume: |
211, Massive Stellar Clusters |
| Page: |
124 |
| Authors: |
Keller, S.; Bessell, M. S.; Da Costa, G. S. |
| Abstract: |
We present the results of our study into the degree of internal mixing within the stellar interior as evident from the population of four young populous clusters in the Magellanic Clouds. Our data shows that it is possible to constrain the degree of convective core overshoot. We consider the illustrative example of NGC 330. Within this cluster we can rule out the case of no convective core overshoot to a 2 sigma level. |
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