The Origin of the Elements in the Milky Way and Its Closest Neighbors

银河系及其最近邻元素的起源

• 批准号: 2307621
• 负责人: David Weinberg
• 金额: $ 45.74万
• 依托单位: Ohio State 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=2307621&HistoricalAwards=false
• 关键词: Origin; Elements; Milky; Way; Its

Understanding the origin and distribution of the elements is essential for understanding the processes that govern galaxy formation. This research project comprises a program of data analysis and modeling to interpret the elemental abundance patterns of stars in the Milky Way and its dwarf satellite galaxies observed by large spectroscopic surveys. Results from the project will allow astronomers to build a coherent picture of stellar and galactic scale phenomena that govern the synthesis of the elements. The project will train a graduate student in methods of advanced astronomical analysis and support a program of research mentoring for undergraduate students.Building upon models developed by the research team, the studies undertaken will yield strong empirical constraints on the contributions of core collapse supernovae, Type Ia supernovae, and asymptotic giant branch stars to the observed stellar elemental abundance patterns. They will provide stringent tests of Milky Way chemical evolution models that explore different assumptions about accretion and star formation history, galactic winds, fountains, radial gas flows, and stochastic enrichment events, as well as incomplete mixing in the interstellar medium. They will also yield new insights on the origin of chemical abundance differences between the components of the Milky Way (thin disk, thick disk, bulge, halo) and between the Milky Way and its dwarf satellites.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.

了解元素的起源和分布对于理解控制星系形成的过程至关重要。该研究项目包括一个数据分析和建模程序，用于解释大型光谱调查观测到的银河系及其矮卫星星系中恒星的元素丰度模式。该项目的结果将使天文学家能够对控制元素合成的恒星和银河尺度现象建立一个连贯的图像。该项目将培训研究生高级天文分析方法，并支持本科生研究指导计划。基于研究团队开发的模型，所进行的研究将对核心塌缩超新星、Ia型超新星和渐近巨分支星对观测到的恒星元素丰度模式的贡献产生强有力的实证约束。他们将对银河系化学演化模型进行严格的测试，探索有关吸积和恒星形成历史、银河风、喷泉、径向气流和随机富集事件以及星际介质中不完全混合的不同假设。他们还将对银河系各组成部分（薄盘、厚盘、核球、晕）之间以及银河系与其矮卫星之间的化学丰度差异的起源产生新的见解。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。