RUI: Interstellar Matter Near the Pleiades: Probing the Cloud-Cluster Interaction with Interstellar Absorption Lines

RUI：昴宿星团附近的星际物质：探索云团与星际吸收线的相互作用

• 批准号: 9117136
• 负责人: Richard White
• 金额: $ 6.14万
• 依托单位: Smith College
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 1991
• 资助国家: 美国
• 起止时间: 1991-12-01 至 1996-11-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9117136&HistoricalAwards=false
• 关键词: RUI; Interstellar; Matter; Near; Pleiades

Recent research has demonstrated that the nebulosity surrounding the familiar Pleiades star cluster results from an accidental encounter between the cluster and an interstellar cloud. Data from the Infrared Astronomical Satellite have revealed the wake of the Pleiades in the ambient interstellar medium, and have indicated the existence of a bow shock where heated gas near the cluster compresses the upstream material. Dr. White's research has the following aims: to trace the motions of the interstellar gas observed toward the Pleiades, particularly in the cluster-cloud interaction region; to explore the physical conditions that prevail in the gas and infer the spatial relationships among the stars and the nearby gas; to characterize interstellar processes in the cluster, particularly the dominant process of gas heating by photoelectrons emitted from dust grains and the poorly understood formation process of the CH+ molecule. The means to these ends will be analysis of interstellar absorption lines in high resolution, high sensitivity spectra of cluster and background stars to be obtained at Kitt Peak National Observatory. This award is made under the Research in Undergraduate Institutions (RUI) program.

最近的研究表明，围绕着我们熟悉的昴宿星团的星云是星团和星际云之间偶然相遇的结果。来自红外天文卫星的数据揭示了昴星团在周围星际介质中的尾迹，并表明在星团附近加热的气体压缩上游物质的弓形激波的存在。怀特博士的研究有以下目标：追踪观测到的朝向昴星团的星际气体的运动，特别是在星团-云相互作用区域；探索气体中普遍存在的物理条件，推断恒星与附近气体之间的空间关系；来描述星系团中的星际过程，特别是由尘埃颗粒发射的光电子加热气体的主要过程和鲜为人知的CH+分子的形成过程。实现这些目标的手段将是分析基特峰国家天文台获得的高分辨率、高灵敏度的星团和背景恒星光谱的星际吸收线。该奖项是在本科院校研究（RUI）项目下颁发的。