Research Areas
He is a computational astrophysicist. His work includes the development of multi-physics, high-order Godunov codes with adaptive mesh capability for massively parallel machines using traditional CPUs and latest GPUs. He uses large-scale computer simulation to study the formation of filamentary structures in highly supersonic and magnetized molecular clouds, what leads to the formation of dense cores, the formation of protostars and the mechanisms of proto-stellar outflows. He also studies the formation of star clusters and their radiation feedback to the molecular cloud environment. He also involves in interpreting and comparison of observational results obtained by the star formation group in SHAO.
