The History of the Milky Way from the Chemodynamics of its Stellar Populations

从恒星族群的化学动力学看银河系的历史

• 批准号: 2755723
• 金额: --
• 依托单位: Liverpool John Moores University
• 依托单位国家: 英国
• 项目类别: Studentship
• 财政年份: 2022
• 资助国家: 英国
• 起止时间: 2022 至 无数据
• 项目状态: 未结题
• 来源: https://gtr.ukri.org/projects?ref=studentship-2755723
• 关键词: History; Milky; Way; Chemodynamics; its

The goal of this thesis is to constrain the mass assembly history of the Milky Way through study of the chemodynamics of its stellar populations. The study will be based on kinematics and chemical data extracted from a combination of the Gaia satellite, SDSS/APOGEE, SDSS/Milky Way Mapper, and WEAVE. The first step will consist of an analysis of the stellar population content as well as structural and kinematic properties of M54, which is the nuclear cluster of the Sgr dSph galaxy. This initial "ice-breaker" project is aimed at familiarizing the PhD candidate with the data and methods employed in the field of Galactic Archaeology, with the goal to deliver a publication within the next year. This analysis will be based on a combination of APOGEE and MUSE data. Upon conclusion of this project the PhD candidate will start the analysis of a combination of WEAVE and SDSS data on halo stellar populations, to constrain the accretion history of the Milky Way.

本论文的目标是通过研究银河系中恒星群体的化学动力学来约束银河系的质量聚集历史。这项研究将基于从盖亚卫星、SDSS/APOGEE、SDSS/银河系绘图仪和WEAVE组合中提取的运动学和化学数据。第一步将包括分析恒星的人口内容以及M54的结构和运动学特性，M54是Sgr dSph星系的核团。这个最初的“破冰船”项目旨在使博士候选人熟悉银河系考古学领域的数据和方法，目标是在明年内发表论文。该分析将基于APOGEE和MUSE数据的组合。该项目结束后，博士候选人将开始分析WEAVE和SDSS关于晕恒星种群的数据，以限制银河系的吸积历史。