Collaborative Research: The Destruction and Growth of Halo Clouds

合作研究：晕云的破坏和增长

• 批准号: 2307693
• 负责人: Mary Putman
• 金额: $ 39.98万
• 依托单位: Columbia University
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2023
• 资助国家: 美国
• 起止时间: 2023-09-01 至 2026-08-31
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2307693&HistoricalAwards=false
• 关键词: Collaborative; Research; Destruction; Growth; Halo

In order for a galaxy to form new stars, the galaxy gathers more hydrogen gas. This gas is thought to rain down onto the galaxy, and indeed, gas clouds of different shapes and sizes are already found around the Milky Way galaxy. Because we see a single snapshot in time, the fate of these gas clouds is not actually known. This project will determine whether the hydrogen clouds grow as they fall into the galaxy as star formation fuel, or if the clouds will be scattered and destroyed as they fall. The investigators will compare computer simulations of clouds moving towards a galaxy to new observations of clouds near the Milky Way. Students will be trained how to conduct scientific research, and the observations will be shared with the public. The physical processes behind the destruction and growth of cool gas clouds in a hot medium is a long standing astrophysical problem. An ideal testing ground for recent theoretical advances is in our own Milky Way, in particular in the halo of our Galaxy, where discrete clouds can be easily isolated, are largely separate from the process of star formation, and are well observed. Detailed comparisons will be made, in the observational plane, of new high-resolution observations of halo clouds to high-fidelity magnetohydrodynamic simulations of the cloud destruction and growth. To complete the comparison between the simulations and observations, a library of simulated clouds with varying physical conditions will be created, and a suite of observational data on clouds with distance constraints will be prepared. The simulated clouds will be put onto the observational plane to compare the spatial morphologies and velocity structures. In addition to the research experiences for students, the project will develop a science service learning course that will teach undergraduates better methods for explaining scientific research to the local community.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.

为了形成新的恒星，星系会聚集更多的氢气。 这种气体被认为会像雨一样落在银河系上，事实上，在银河系周围已经发现了不同形状和大小的气体云。 因为我们看到的是一张时间快照，这些气体云的命运实际上并不知道。这个项目将确定氢云是在作为星星形成燃料落入星系时生长，还是在下落时被分散和破坏。 研究人员将把计算机模拟的云向星系移动的过程与对银河系附近云的新观测结果进行比较。 学生将接受如何进行科学研究的培训，观察结果将与公众分享。 在热介质中冷气体云的破坏和增长背后的物理过程是一个长期存在的天体物理问题。最近理论进展的一个理想的试验场是在我们自己的银河系，特别是在我们银河系的晕中，在那里离散的云可以很容易地分离出来，在很大程度上与星星形成的过程分开，并且被很好地观察到。在观测平面上，将对晕云的新的高分辨率观测与云的破坏和增长的高保真磁流体动力学模拟进行详细的比较。 为了完成模拟和观测之间的比较，将建立一个具有不同物理条件的模拟云库，并准备一套关于具有距离限制的云的观测数据。 将模拟的云放在观测平面上，比较云的空间形态和速度结构。除了为学生提供研究经验外，该项目还将开发一门科学服务学习课程，教授本科生更好地向当地社区解释科学研究的方法。该奖项反映了NSF的法定使命，并通过使用基金会的智力价值和更广泛的影响审查标准进行评估，被认为值得支持。