Growing galaxies: a consistent view of star formation across cosmic time

成长中的星系：整个宇宙时间恒星形成的一致观点

• 批准号: FT150100079
• 负责人: A/Prof Elisabete da Cunha
• 金额: $ 49.74万
• 依托单位: The University of Western Australia
• 依托单位国家: 澳大利亚
• 项目类别: ARC Future Fellowships
• 财政年份: 2016
• 资助国家: 澳大利亚
• 起止时间: 2016-05-01 至 2023-04-30
• 项目状态: 已结题
• 来源: https://dataportal.arc.gov.au/RGS/Web/Grants/FT150100079
• 关键词: Growing; galaxies; consistent; view; star

The project aims to contribute to the answer to a fundamental question: how galaxies, including our own, evolved over the Universe's history. The project plans to develop sophisticated spectral models and use them to extract crucial information on star formation, stellar populations, interstellar gas and dust properties from modern galaxy surveys at different cosmic epochs using a consistent framework. These imaging and spectroscopic surveys would be complemented with measurements of the total gas reservoir of galaxies, obtaining a full census of the baryons in galaxies. Together, these may deliver significant insights into how the growth of galaxies, driven by the fuelling, efficiency and outputs of star formation, depends on galaxy properties in the local and distant Universe.

该项目旨在为一个基本问题的答案做出贡献：包括我们自己的星系如何在宇宙的历史中发展。该项目计划开发复杂的光谱模型，并使用它们来提取有关恒星形成，恒星种群，星际气体和灰尘特性的关键信息，并使用一致的框架在不同的宇宙时代的现代星系调查中提取恒星形成，尘埃落定。这些成像和光谱调查将与银河系总气体库的测量相辅相成，并在星系中获得了巴属的完整普查。总之，这些可能会对星系生长的加油，效率和恒星形成的产量的驱动如何取决于局部和遥远宇宙中的星系特性。