About
Se-Heon Oh is a Professor in the Department of Physics and Astronomy at Sejong University, specializing in galaxy dynamics, observational radio astronomy, and dark matter studies. His work bridges theoretical and empirical approaches to understanding galactic evolution.
Education:
- Ph.D., The Australian National University (2009)
- B.S., Yonsei University (2004)
Research Interests: Galaxy dynamics linked to star formation, observational radio astronomy focusing on H i gas, and galaxy surveys using SKA pathfinders. His studies explore dark matter profiles in dwarf galaxies and precision kinematic measurements for large-scale surveys.
Recent Publications (2025): Cutting-edge work on H i gas dynamics, turbulent gas accretion in M51, and star formation in gas-rich galaxy pairs, showcasing his focus on galactic feedback mechanisms and environmental impacts.
Collaborations: Active in international projects like WALLABY, MHONGOOSE, and THINGS, working with institutions across Australia, South Africa, and the U.S. using telescopes like MeerKAT and VLA.
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