The Three-Dimensional Structure of the Milky Way

银河系的三维结构

• 批准号: 9117388
• 负责人: David Spergel
• 金额: $ 15万
• 依托单位: Princeton University
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 1992
• 资助国家: 美国
• 起止时间: 1992-02-15 至 1995-07-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9117388&HistoricalAwards=false
• 关键词: Three; Dimensional; Structure; Milky; Way

The goal of Dr. Spergel's project is to synthesize the growing body of observational data that suggests that our Galaxy, the Milky Way, has significant non-axisymmetric structure. Improvements in infrared technology have enabled astronomers to observe the galactic center at wavelengths not obscured by dust. These observations suggest that our Galaxy is barred. Radio wavelength surveys of gas motions in our Galaxy reveal significant non- circular motions that are likely due to this bar. Dr. Spergel plans to develop analytical and numerical techniques to construct a three-dimensional model of the Milky Way that is consistent with the observations. Improvements in our understanding of orbital dynamics in triaxial systems as well as improvements in numerical techniques and computer hardware will facilitate this study. Dr. Spergel also plans to study the dynamics of corrugation waves and spiral density waves excited by the bar and the galactic spheroid and to explore how these waves alter gas motions in the Galaxy. Ultimately the goal of this research is to better understand the morphology and dynamics of the Milky Way and to provide insight into its origin and evolution.

Spergel博士项目的目标是综合不断增长的观测数据，这表明我们的银河系是银河系具有重要的非轴对称结构。 红外技术的改进使天文学家能够在未被灰尘遮盖的波长下观察银河系中心。 这些观察结果表明我们的星系被禁止。 我们银河系中气体运动的无线电波长调查显示出可能归因于该条的明显的非圆形运动。 Spergel博士计划开发分析和数值技术，以构建与观测值一致的银河系模型的三维模型。 我们对三轴系统轨道动态的理解以及数值技术和计算机硬件的改进将有助于这项研究的改进。 Spergel博士还计划研究横杆和银河球体激发的波纹波和螺旋密度波的动力学，并探索这些波如何改变星系中的气体运动。 最终，这项研究的目的是更好地了解银河系的形态和动态，并提供对其起源和进化的见解。