金属丰富的球状星团和金属贫乏的球状星团之间的年龄差异为20亿年
B M S Hansen1, J S Kalirai, J Anderson
1Division of Astronomy, University of California Los Angeles, Los Angeles, California 90095, USA. hansen@astro.ucla.edu
球状星团揭示了星系形成的历史. 金属丰富的球状星团47 Tucanae年龄为99亿年,比NGC 6397.7等金属贫富星团晚形成.
科学领域:
- 天文学和天体物理学
- 银河系考古学 银河系考古学
- 恒星进化 恒星进化
背景情况:
- 球状星团对于理解星系的形成和演变至关重要.
- 星团金属性和年龄为银河系组成部分的形成序列提供了洞察力.
- 在银河系的光环中发现了金属贫困的星团,而金属丰富的星团则位于内部区域.
研究的目的:
- 确定富含金属的球状星团47 Tucanae的绝对年龄.
- 为了比较金属丰富和金属贫乏的球状星团的形成时间.
- 为银河系组件形成的序列提供定量证据.
主要方法:
- 模拟球状星团的白矮冷却序列.
- 利用恒星群体的精确年龄测定技术.
- 对不同金属度集群之间的年龄数据进行比较分析.
主要成果:
- 富含金属的球状星团47 Tucanae的绝对年龄为9.9 ± 0.7亿年.
- 这个年龄大约比金属贫困星团NGC 6397.7年轻20亿年.
- 定量证据表明,金属丰富的星团比金属贫富的光环星团晚形成.
结论:
- 像47 Tucanae这样的金属丰富的球状星团比NGC 6397.7.这样的金属贫乏的光环星团形成晚.
- 这种年龄差异支持银河系组件的顺序形成模型.
- 球状星团年龄是星系层次组合的关键标志物.
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