Welcome to Prof. Sukyoung K. Yi's group (GEM) homepage

The ultimate goal of our group is to understand the formation and evolution of galaxies. We work on various versions of galaxy formation theories, focusing on dynamical clustering of galaxies and galactic chemical evolution in combination with stellar population synthesis. We extensively, but not exclusively, use SDSS and GALEX data to test our theoretical models.

The 3rd GEM-Jeju workshop on the formation of large galaxies will be held at Shilla, Jeju on 21-24 January. Further details of the workshop are presented in this website.

Title: Merger relics of cluster galaxies

Explanation: Merger Relics of Cluster Galaxies. Merger features are found too often in massive cluster galaxies to be fully explained by in-situ galaxy mergers that are theoretically thought to be rare in such deep potential wells. We attempted to explain this new observational finding (Sheen et al. 2012) using numerical simulations in combination with semi-analytic approach of galaxy formation theory. We found that mergers last so very long in deep observing conditions that many of the merger-featured galaxies in present-day clusters may have originated from the mergers in their previous halo environments, hence the name "merger relics". Published in Astronomy and Astrophysics (15 June 2013).
Full text [ADS]

Seulhee Oh has been awarded "The best publication award". Yonsei has chosen her bar galaxy paper as one of the 6 best papers published in 2011 by Yonsei students. Congratulations!

Last modified: 2014-01-29
   Since 25 March 2010
Dept. of Astronomy, Yonsei University
134 shinchon-dong, Sudaemun-gu, Seoul 120-179 Korea
Copyright 2006 Galaxy Evolution Meeting. Maintained by J. Lee