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含量作为球状星团恒星的先进进化的预测因素

Simon W Campbell1, Valentina D'Orazi, David Yong

  • 1Monash Centre for Astrophysics, School of Mathematical Sciences, Monash University, Melbourne, Victoria 3800, Australia. simon.campbell@monash.edu

Nature
|May 31, 2013
PubMed
概括

在NGC 6752球状星团中的第二代恒星没有达到非对称巨分支 (AGB) 阶段,这与恒星进化预测相反. 这一发现挑战了使用AGB恒星来测试星团中的恒星进化时间表的使用.

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