Probing the Nature and Origin of Ultra Diffuse Galaxies (UDGs) with Deep and Wide-Field Imaging

利用深视场和广视场成像探测超漫射星系 (UDG) 的性质和起源

• 批准号: 1812847
• 负责人: Jin Koda
• 金额: $ 48.7万
• 依托单位: SUNY at Stony Brook
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2018
• 资助国家: 美国
• 起止时间: 2018-06-15 至 2023-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1812847&HistoricalAwards=false
• 关键词: Probing; Nature; Origin; Ultra; Diffuse

Ultra-diffuse galaxies (UDGs) are a newly discovered population of galaxies. They are extremely faint, but spatially very extended, and are almost blended in the brightness of the night sky. Such diffuse galaxies are fragile, and cannot survive in gravitational encounters with other galaxies. However, astronomers are finding a great number of UDGs in clusters of galaxies, where such encounters would occur. This research program will investigate the nature and origin of these UDGs. It will study (1) whether UDGs are distinct from other types of galaxies such as the Milky Way and dwarf galaxies; (2) how they are protected from the gravitational disruptions; and (3) whether they have even fainter outskirts. The effects of gravitational encounters should appear clearly in the outskirts. This project will engage a variety of students in the research.This program will use deep and wide-field imaging of eight local clusters of galaxies. The data are taken with the Hyper Suprime-Cam (HSC) on the Subaru telescope. These unique data will show the very faint outskirts of UDGs, as well as their large-scale environments. The program will perform the most reliable census and resolved analysis of the UDG population within, outside, and among the clusters. The main goals are (1) to confirm whether UDGs are distinct from dwarf and normal galaxies in their properties parameter spaces; (2) to constrain how they formed and how they their properties depend on their environments; and (3) to image their fainter outskirts and to discover even fainter, more extended UDGs. The project focuses primarily on UDGs, but aims to yield a broader, coherent picture that connects UDGs, dwarfs, and normal galaxies. UDGs are faint and extended, and are difficult to be detected and analyzed. The observations and data reduction will be optimized to achieve these goals.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

超扩散星系（UDG）是一个新发现的星系群。它们非常微弱，但在空间上非常延伸，几乎与夜空的亮度融为一体。这样的弥漫星系是脆弱的，在与其他星系的引力相遇中无法生存。然而，天文学家在星系团中发现了大量的UDG，在那里会发生这种遭遇。本研究计划将调查这些UDG的性质和起源。它将研究（1）UDG是否与其他类型的星系（如银河系和矮星系）不同;（2）它们如何免受引力破坏的影响;以及（3）它们是否有更暗的外围。引力相遇的影响应该会在郊区清晰地显现出来。这个项目将吸引各种各样的学生参与研究。这个项目将使用八个本地星系团的深视场成像。这些数据是用斯巴鲁望远镜上的超级超级凸轮（HSC）拍摄的。这些独特的数据将显示UDG非常微弱的外围以及它们的大规模环境。该计划将执行最可靠的人口普查和解决分析的UDG人口内，外，和集群之间。主要目标是：（1）确认UDG在其性质参数空间中是否与矮星系和正常星系不同;（2）限制它们如何形成以及它们的性质如何取决于它们的环境;（3）对它们较暗的外围进行成像，并发现更暗，更扩展的UDG。该项目主要关注UDG，但旨在产生一个更广泛的，连贯的图片，连接UDG，矮星和正常星系。UDG是一种模糊的、扩展的、难以检测和分析的特征。该奖项反映了NSF的法定使命，并通过使用基金会的知识价值和更广泛的影响审查标准进行评估，被认为值得支持。