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Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
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银河系早期形成的时间解析图
Maosheng Xiang1, Hans-Walter Rix2
1Max-Planck Institute for Astronomy, Koenigstuhl 17, Heidelberg, Germany. mxiang@mpia.de.
Nature
|March 24, 2022
概括
我们的银河系
科学领域:
- 天文学与天体物理学
- 银河系考古学
- 恒星进化
背景情况:
- 银河系的形成涉及不同的阶段,创造了它的光环和圆盘恒星群.
- 了解银河系组合需要从大样本中精确的恒星年龄.
研究的目的:
- 通过精确的子巨星年龄量化分析银河系的形成历史.
- 解决银河系光环和磁盘组成部分的不同形成阶段.
主要方法:
- 分析了一大批具有精确年龄测量的小巨星.
- 对恒星年龄-金属度分布的检查p{\displaystyle p} ,[Fe/H]).
主要成果:
- 恒星年龄金属度分布分为两个群体,大约为8 Gyr.
- 一个年轻的群体表明静止的银河系盘形成与辐射迁移.
- 一个较老的群体揭示了恒星光环和厚盘的形成.
结论:
- 旧的,厚的磁盘形成大约13年,大爆炸后不久.
- 盖亚-香肠-恩塞拉多斯的合并大约11个Gyr前显著影响了恒星形成.
- 银河系在最初的形成后进行了连续的化学丰富.
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