Fundamental Modes of Galaxy Formation Through Cosmic Time

宇宙时间中星系形成的基本模式

• 批准号: 1108815
• 负责人: Michael Rauch
• 金额: $ 24.66万
• 依托单位: Carnegie Institution of Washington
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2011
• 资助国家: 美国
• 起止时间: 2011-09-01 至 2015-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1108815&HistoricalAwards=false
• 关键词: Fundamental; Modes; Galaxy; Formation; Through

Galaxies are thought to form primarily through the merging of smaller galaxies and the accretion of cold gas from the intergalactic medium (IGM). The aim of this project is to directly detect the low mass building blocks of present-day galaxies like the Milky Way and the signatures of gas transport from the IGM into gaseous halos and disks. The collaborating team will make use of spectroscopic observations that can provide higher contrast between faint galaxies and the sky background than broad- or narrow-band imaging, and will take advantage of recent increases in instrumental sensitivity and their access to large telescopes. The team will carry out 4 distinct sub-projects: (1) Spectroscopic searches for Lyman-alpha emission from the IGM and high redshift galaxies. The aim is to reveal the spatial extent, kinematics and energetics of gas in the early stages of galaxy formation. (2) Line-profile analysis of bright Lyman-alpha galaxies. The data will be used to constrain the relative importance of infall and outflow in galaxies. (3) High resolution spectroscopy of MgII absorption systems in the spectra of background quasi-stellar objects (QSOs). These data will be used to understand the origin of cool gas clouds in galaxies without current star formation. (4) A deep, two-dimensional Balmer-alpha search of local galaxies in an effort to detect cool halo clouds condensing from the halo onto the disk. These projects are intended to be available as doctoral dissertation projects for graduate students in the Carnegie Institution's pre-doctoral fellowship program. The Principal Investigator will also participate in supervising undergraduate students from the Claremont Colleges in astronomy research.

星系团被认为主要是通过较小星系的合并和星系际介质（IGM）的冷气体的吸积形成的。该项目的目的是直接探测像银河系这样的现代星系的低质量构建块，以及从IGM到气态晕和盘的气体传输的特征。合作团队将利用光谱观测，这种观测可以提供比宽带或窄带成像更高的微弱星系和天空背景之间的对比度，并将利用最近仪器灵敏度的提高及其对大型望远镜的访问。该小组将开展4个不同的子项目：（1）光谱搜索IGM和高红移星系的莱曼α发射。其目的是揭示星系形成早期气体的空间范围、运动学和能量学。(2)明亮莱曼α星系的线轮廓分析。这些数据将用于限制星系中流入和流出的相对重要性。(3)背景类星体光谱中MgII吸收系统的高分辨光谱学。这些数据将用于了解没有当前星星形成的星系中冷气体云的起源。(4)一个深入的，二维的巴耳末-阿尔法搜索本地星系，努力检测冷晕云冷凝从晕到磁盘。这些项目旨在作为卡内基研究所博士前奖学金项目的研究生的博士论文项目。首席研究员还将参与指导克莱蒙学院的本科生进行天文学研究。