HL
Hui Li
Tsinghua University, Columbia University, University of Michigan, Nanjing University, Massachusetts Institute of Technology
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Galaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies
0000-0002-1253-2763
Employment
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Tsinghua University Assistant Professor2024 - Present
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Columbia University Hubble Fellow2020 - 2024
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Massachusetts Institute of Technology Hubble Fellow2019 - 2020
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Massachusetts Institute of Technology Research associate2017 - 2019
Education
- 2012 - 2017
- 2009 - 2012
- 2005 - 2009
Projects & Funding
Projects & funding information is unavailable.
Publications (77)
- Individual Star Sampling in Star Formation Simulations: A Semideterministic Model Save
- Divergent Evolution of Radial Metallicity Gradients in the Thin and Thick Disks of the Milky Way Save
- SMUGGLE-Ring: Evolutionary link between nuclear star cluster and nuclear disk Save
- The SMUGGLE-Ring project: Bar and bulge effects on nuclear disk and ring formation Save
- Probing the Hot Gaseous Halos of Milky Way–like Galaxies in the TNG50 Simulation Save
- 3D moving-mesh hydrodynamical simulations of wind-/jet-driven ultraluminous X-ray source bubbles Save
- Identifying Signatures of Inflow onto Face-on Galaxies Using the Balmer Decrement Save
- The thesan project: environmental drivers of Local Group reionization Save
- RIGEL: Feedback-regulated cloud-scale star formation efficiency in a simulated dwarf galaxy merger Save
- The thesan-zoom project: star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts Save
- Transferring Data from a Voronoi Mesh to an Adaptive Cartesian Grid in Pursuit of Self-consistent Top-down Star Formation Save
- Tracing the Origins of Hot Halo Gas in Milky Way–type Galaxies with SMUGGLE Save
- Probing Turbulence, Gravity, Supernovae, and Magnetic Field Effects with the 6D Kinematics of Young Stars in Milky Way Star-forming Regions Save
- N-body Simulations of Galaxy Bars Generated by Satellite Collisions: Effects of the Impact Geometry Save
- The Importance of Tidal Forces in Molecular Cloud Dynamics Save
- The life cycle of giant molecular clouds in simulated Milky Way-mass galaxies Save
- Understanding the baryon cycle: Fueling star formation via inflows in Milky Way-like galaxies Save
- Stellar Streams Reveal the Mass Loss of Globular Clusters Save
- The Star Clusters as Links between Galaxy Evolution and Star Formation Project. I. Numerical Method Save
- Size Growth on Short Timescales of Star-forming Galaxies: Insights from Size Variation with Rest-frame Wavelength with JADES Save