学术活动

[Colloquium] Stijn Wuyts: Structural evolution of galaxies since cosmic noon

发布时间:2023-06-28
 
国台学术报告2023第13次/NAOC Colloquium No.13 2023
   
报告题目/Title Structural evolution of galaxies since cosmic noon /宇宙正午以来的星系结构及演化
报告人/Speaker Prof. Stijn Wuyts (University of Bath)
报告时间/Time Wednesday 2:30 PM, June 28, 2023
报告地点/Location NAOC A601 & Live Streaming on NAOC WeChat Channel
主持人/Host Prof. Yu Dai (NAOC)
报告语言/Language: English/英文
报告海报/Poster Click to get the poster
演示幻灯片/Slides Click to view the details (later)
报告视频/Video Click to watch the video (later) 
直播链接/Live Webcast: 国台微信公众号视频号(微信扫描如下二维码)
   
报告摘要/Abstract  
In this talk he will discuss the geometry, structure and morphological transformation of star-forming and quiescent galaxies from the peak of cosmic star formation to the present day.  Resolved observations from multiple wavelengths and tracers enable us to reconstruct where stars form within galaxies and how stellar distributions are assembled, while simultaneously revealing insights into the evolving 3D spatial distributions of stars and dust.  Integral-field spectroscopy adds to this the kinematic perspective, probing both gravitational and non-gravitational motions, and with it signatures of dark matter content and feedback in action.  He will draw from HST, JWST, ALMA and IFU observations to illustrate the structural make-up of galaxies across cosmic time, and will draw connections to state-of-the-art cosmological simulations. 
   
报告人介绍/Bio:  
Prof. Stijn Wuyts is a Professor of Astrophysics at the University of Bath.  He obtained his PhD from Leiden University on the topic of "Red Galaxies at High Redshift", worked on the interface between galaxy observations and simulations as a Keck Fellow at the Harvard-Smithsonian Center for Astrophysics, and further explored the distant Universe as a Junior Scientist at the Max Planck Institute for Extraterrestrial Physics.  At the University of Bath, he combines tracers of stars, dust, ionized and cold gas to reveal the physics governing the build-up of stars within galaxies near and far, and the evolution of their structure through cosmic time.
   
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