银河系外层的螺旋结构在中
E S Levine1, Leo Blitz, Carl Heiles
1Astronomy Department, University of California, 601 Campbell Hall, Berkeley, CA 94720, USA. elevine@astron.berkeley.edu
概括
这项研究绘制了银河系中性的地图,揭示了一个非轴对称的,多臂螺旋结构,延伸超过25千帕秒. 这张详细的地图为我们银河系提供了新的见解.
科学领域:
- 天文学和天体物理学
- 银河系的动力学
- 星际地图学 星际地图学
背景情况:
- 银河系的大规模结构传统上被建模为轴对称,但对非轴对称特征的观测证据越来越多.
- 了解中性 (HI) 的分布和动态对于绘制螺旋臂和确定银河系盘的范围至关重要.
研究的目的:
- 为了创建一个详细的表面密度图中性在外层银河系的磁盘.
- 为了研究银河系的螺旋结构,并确定其气体盘的辐射范围.
- 描述银河系螺旋臂的特性,包括它们的形状和密度变化.
主要方法:
- 分析观测数据,绘制中性的扰动表面密度.
- 在银河系南半球的螺旋结构的识别和追踪.
- 将对数螺旋模型与观察到的螺旋臂相匹配,以确定俯仰角.
主要成果:
- 确认银河系是一个非轴对称的,多臂螺旋星系.
- 螺旋结构在外盘中清晰地划定,延伸至至少25千帕塞克,为气体盘建立最低半径.
- 中性表面密度的过密度与气体厚度降低的区域相关,沿臂的表面密度比是相对恒定的.
- 逻辑螺旋的斜角在20度和25度之间,准确地适合观察到的螺旋臂.
结论:
- 详细的HI地图提供了强有力的证据,证明银河系外盘中的非轴对称,多臂螺旋结构.
- 气体盘延伸到至少25 kiloparsecs,其结构的特点是密度变化和特定的螺旋臂几何形状.
- 这些发现完善了我们对银河系形态和螺旋星系气体分布的理解.
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