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银河系光环中的两个恒星组成部分
Daniela Carollo1, Timothy C Beers, Young Sun Lee
1INAF-Osservatorio Astronomico di Torino, 10025 Pino Torinese, Italy. carollo@mso.anu.edu.au
Nature
|December 14, 2007
概括
银河系是我们的银河系.
科学领域:
- 天文学和天体物理学
- 宇宙结构的形成宇宙结构的形成
- 银河系进化过程中的银河系进化.
背景情况:
- 银河系的光环包含了关于早期宇宙物体的关键数据.
- 之前的研究表明光环结构存在分歧.
- 这种分歧的证据是基于小样本大小.
研究的目的:
- 为了明确证明银河系的光环可以分为两个不同的组成部分.
- 为了描述这两个光环组成部分之间的差异.
- 推断每个组件的形成机制.
主要方法:
- 空间密度配置文件的分析.
- 对恒星轨道特征的检查.
- 测量恒星的金属性 (重元素的丰度).
主要成果:
- 光环可以清楚地分为内部和外部组成部分.
- 内部光环呈现出渐进的旋转和更高的金属性.
- 外光环显示逆向旋转和较低的金属性 (内光环的三分之一).
结论:
- 这些独特的特性表明,内部和外部光环的形成途径从根本上有所不同.
- 内部光环可能是通过消散性合并形成的.
- 外层光环可能是通过无散射的合并和原银河团的潮破坏而形成的.
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