Distances to high-velocity clouds

到高速云的距离

• 批准号: 0607474
• 负责人: Donald York
• 金额: $ 11.73万
• 依托单位: University of Chicago
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2006
• 资助国家: 美国
• 起止时间: 2006-08-01 至 2010-07-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0607474&HistoricalAwards=false
• 关键词: Distances; velocity; clouds

AST-0607474INSTITUTION: University of ChicagoPI: Donald YorkTITLE: Distances to High-Velocity CloudsABSTRACTDr. Donald York (University of Chicago), along with collaborators Dr. Bastiaan Wakker (University of Wisconsin at Madison), Dr. Timothy Beers (Michigan State University), and Dr. Ronald Wilhelm (Texas Tech University), will undertake a program to determine the distances to 14 so-called high-velocity clouds (HVCs), and intermediate-velocity clouds" (IVCs). These are massive clouds of neutral hydrogen gas that are moving with velocities that are incompatible with simple models of galactic rotation. The goal will be accomplished by first determining the distances to blue horizontal branch" (BHB) stars along the line of sight from medium-resolution spectra, and then looking for interstellar absorption features from the clouds in high-resolution spectra. By determining which spectra reveal the signature of the clouds, and knowing the distances to the stars from which the spectra were derived, constraints on distances to the clouds can be obtained. Distances to these clouds remain one of the outstanding problems in Galactic astronomy, and resolution of the nature of these clouds will provide important constraints on models of galaxy formation and evolution.The work will have broad impact on various sub-fields of astronomy, particularly galaxy formation and evolution. Components of the program are self-contained, and well-suited for graduate and undergraduate research projects. Outreach activities will also be undertaken.

AST-0607474机构：芝加哥大学PI：Donald York标题：到高速云的距离摘要Dr.唐纳德约克（芝加哥大学），沿着合作者巴斯蒂安·瓦克博士（威斯康星州麦迪逊大学），蒂莫西·比尔斯博士（密歇根州立大学），和罗纳德·威廉博士（得克萨斯理工大学），将进行一项计划，以确定14个所谓的高速云（HVC）和中速云（IVC）的距离。 这些是巨大的中性氢气云，其移动速度与简单的星系旋转模型不相容。 这一目标将通过以下方法实现：首先从中等分辨率光谱中确定沿视线沿着到蓝色水平分支星（BHB）的距离，然后从高分辨率光谱中的云中寻找星际吸收特征。 通过确定哪些光谱揭示了云的特征，并知道到光谱所来源的恒星的距离，可以获得到云的距离的约束。这些云的距离仍然是银河系天文学中的一个突出问题，而这些云的性质的解决将为星系形成和演化的模型提供重要的约束条件，这项工作将对天文学的各个子领域，特别是星系的形成和演化产生广泛的影响。该计划的组成部分是独立的，非常适合研究生和本科生的研究项目。 还将开展外联活动。