Young populous clusters in the magellanic clouds

被引：0
|
作者：
Keller, S [1 ]
Bessell, MS [1 ]
Da Costa, GS [1 ]
机构：
[1] Res Sch Astron & Astrophys, Weston Creek PO, ACT 2611, Australia
来源：
MASSIVE STELLAR CLUSTERS | 2000年 / 211卷
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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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页码：124 / 127
页数：4
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