
摘要
Hot gas plays a vital role in shaping galaxy formation and evolution. However, even though we live in a disk galaxy, we know very little about the distribution of this hot gas, and how it impacts the disk galaxy evolution via the so-called “circumgalactic medium”. In this talk, I will discuss several outstanding questions in this field, including problems such as the “missing galactic baryons” and “missing stellar feedback”. I will also discuss how addressing these questions can help understand galaxy formation and evolution processes in general, as well as the baryonic matter distribution in the universe.
报告人简介
方陶陶,厦门大学天文系教授,物理科学与技术女王调教 院长兼天文系系主任。武汉大学本科,中国科技大学硕士,美国麻省理工女王调教 博士。主要研究方向为宇宙大尺度结构、星系形成和演化。获美国 NASA Chandra Fellow、中国国家基金委杰出青年等。
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