Chia-Yu Hu

The IllustrisTNG simulations: public data release

Properties of galaxies reproduced by a hydrodynamic simulation

Theoretical Challenges in Galaxy Formation

The kinematics and dark matter fractions of TNG50 galaxies at z = 2 from an observational perspective

How to model supernovae in simulations of star and galaxy formation

Mass transfer in white dwarf–neutron star binaries

The Fate of Binaries in the Galactic Center: The Mundane and the Exotic

Accurate, meshless methods for magnetohydrodynamics

Physics-informed neural networks for high-speed flows

Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe

A new multi-resolution parallel framework for SPH

Galaxies on FIRE (Feedback In Realistic Environments): stellar feedback explains cosmologically inefficient star formation

Modeling the Atomic-to-molecular Transition in Cosmological Simulations of Galaxy Formation

The Galaxy in Context: Structural, Kinematic, and Integrated Properties

First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations

First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback

Simulating galaxy formation with the IllustrisTNG model

The impact of mechanical AGN feedback on the formation of massive early-type galaxies

SPHGal: smoothed particle hydrodynamics with improved accuracy for galaxy simulations

Star formation and molecular hydrogen in dwarf galaxies: a non-equilibrium view

Variable interstellar radiation fields in simulated dwarf galaxies: supernovae versus photoelectric heating

Supernova-driven winds in simulated dwarf galaxies