The Chemical Compositions of Galactic Halo Field and Cluster Stars

银河晕场和星团的化学成分

• 批准号: 0908978
• 负责人: Christopher Sneden
• 金额: $ 26.27万
• 依托单位: University of Texas at Austin
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2009
• 资助国家: 美国
• 起止时间: 2009-08-01 至 2013-07-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0908978&HistoricalAwards=false
• 关键词: Chemical; Compositions; Galactic; Halo; Field

This award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5).Two major surveys of Galactic field halo stars will be carried out in order to illuminate and constrain models of early chemical evolution in the Milky Way Galaxy. In one, a detailed study of high resolution spectra of over 100 stars with known space motions and metallicities less than 1/300 that of the sun will be undertaken, with the goal of discovering abundance trends with kinematic properties of the stars. The second is a comprehensive survey of very evolved so-called horizontal branch stars using multi-object spectra of about 10 globular clusters. The Broader Impacts of this program include dissemination of computer codes and atomic line data to the astronomical community, and participation in a program involving secondary school teachers.

该奖项是根据2009年美国复苏和再投资法案（公法111-5）资助的。将进行两次银河系场晕星的主要调查，以照亮和约束银河系早期化学演化的模型。 其中一个项目将详细研究100多颗已知空间运动和金属丰度不到太阳1/300的恒星的高分辨率光谱，目的是发现恒星运动学特性的丰度趋势。 第二个是使用大约10个球状星团的多目标光谱对非常演化的所谓水平分支恒星进行全面调查。 该计划的更广泛影响包括向天文学界传播计算机代码和原子线数据，以及参与一个涉及中学教师的计划。