From Clusters to Voids: Gas and Galaxy Evolution

从星团到空洞：气体和星系演化

• 批准号: 1009476
• 负责人: Jacqueline van Gorkom
• 金额: $ 41.89万
• 依托单位: Columbia University
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2010
• 资助国家: 美国
• 起止时间: 2010-09-15 至 2014-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1009476&HistoricalAwards=false
• 关键词: Clusters; Voids; Gas; Galaxy; Evolution

This project consists of three complementary observational efforts, intended to test the conceptual picture that galaxies may gain mass from their surroundings not by accretion of hot plasma that cools as it settles into the galaxy, but rather by accretion of gas that has already cooled in the intergalactic environment and remains cold as it flows into the galaxy, possibly on orderly streams with preferred directions. This idea has gained theoretical support in recent years through hydrodynamical simulations of galaxy formation; observational tests to be performed by the PI consist of radio observations, primarily in the 21 cm neutral hydrogen line, of (1) the outer parts of the nearby Virgo cluster of galaxies, (2) large volumes surrounding two distinctly different clusters at redshift z=0.2, and (3) galaxies located in extremely under-dense void regions. This work will exploit the newly enhanced capabilities of the Westerbork Synthesis Radio Telescope (WSRT) in the Netherlands and the Expanded Very Large Array (EVLA) in the US. The new data will be combined with archived data to compare the morphologies, star forming properties, environments, and (where appropriate) locations within the clusters of galaxies with, and without, spatially extended cold gas. The observations will be compared against predictions made by high-resolution hydrodynamical simulations performed by a collaborator on the project; and the Virgo observations, in particular, will be made available to the research community through a website. The work will involve the participation of undergraduate and graduate students from under-represented groups, and will be highlighted in public presentations in schools and other venues.

该项目包括三项相辅相成的观测工作，旨在检验星系从其周围环境获得质量的概念图景，即星系可能不是通过吸积热等离子体而获得质量，热等离子体在进入星系时冷却，而是通过吸积在星系间环境中已经冷却并在流入星系时保持低温的气体，可能是以具有优先方向的有序流。这一想法近年来通过星系形成的流体动力学模拟获得了理论支持;由PI进行的观测测试包括射电观测，主要是在21厘米中性氢线上，观测（1）附近室女座星系团的外部，（2）红移z=0.2的两个明显不同的星系团周围的大体积，（3）位于极低密度空洞区域的星系。这项工作将利用荷兰Westerbork综合射电望远镜（WSRT）和美国扩展甚大阵列（EVLA）的新增强功能。新的数据将与存档的数据相结合，以比较形态，星星形成特性，环境和（在适当的情况下）在星系团内的位置，以及没有空间扩展的冷气体。观测结果将与该项目的一名合作者进行的高分辨率流体动力学模拟所作的预测进行比较;特别是Virgo观测结果将通过一个网站提供给研究界。这项工作将涉及来自代表性不足群体的本科生和研究生的参与，并将在学校和其他场所的公开演讲中突出强调。