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射手座的影响作为螺旋和银河系外环的建筑师
Chris W Purcell1, James S Bullock, Erik J Tollerud
1Department of Physics and Astronomy, The University of Pittsburgh, Pittsburgh, Pennsylvania 15260, USA. cpurcell@pitt.edu
Nature
|September 17, 2011
概括
银河系的螺旋臂和条形结构可能不是完全自我生成的. 模拟显示,射手座矮星系的撞击显著塑造了银河系形态,包括螺旋臂和磁盘燃烧.
科学领域:
- *银河系动力学和天体物理学.
- *计算天体物理学和星系形成.
背景情况:
- *银河系的结构,包括其螺旋臂和中心条,尚未完全理解.
- *以前的模型通常假定银河系形态学上的外部影响最小.
- *小聚合在塑造星系结构中的作用是一个正在进行的研究领域.
研究的目的:
- *为了模拟银河系对射手座矮星系 (Sgr) 撞击的反应.
- * 调查这种小型合并对银河系形态学的影响,包括螺旋臂,中心条和圆盘.
- * 评估外部力量对银河系结构的贡献,特别是小规模的合并.
主要方法:
- *N体模拟模拟了银河系和射手座矮星系之间的引力相互作用.
- *对模拟输出进行分析,以观察银河系结构的变化,例如螺旋臂形成和磁盘燃烧.
- * 将模拟结果与银河系特征的观测数据进行比较.
主要成果:
- * 射手座矮星系的入引发了突出螺旋臂的形成.
- * 中央条结构受到影响,产生了膨胀的外盘.
- *向银河系反中心观察到两个环状的包裹,与观测到的弧形一致.
结论:
- *银河系的形态不仅仅是世俗的起源;外部影响是显著的.
- * 像Sgr撞击这样的微小合并,在塑造银河系结构方面发挥着至关重要的作用.
- *这些发现表明,在整个宇宙的星系进化中,微小的合并很重要.
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