78 Papers
349 Citations
Hui Li is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Solar wind & Interplanetary magnetic field. The author has an hindex of 16, co-authored 63 publications. Previous affiliations of Hui Li include University of Science and Technology of China & North China University of Water Conservancy and Electric Power.
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Papers
Modeling the Formation of Globular Cluster Systems in the Virgo Cluster
Hui Li,Oleg Y. Gnedin +1 more
TL;DR: In this article, a simple model for the formation and disruption of globular cluster (GC) systems is presented, which aims to match the ACSVCS data and test the hypothesis that GCs are formed during major mergers of gas-rich galaxies and inherit the metallicity of their hosts.
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Star cluster formation in cosmological simulations. i. properties of young clusters
Hui Li,Oleg Y. Gnedin,Nickolay Y. Gnedin,Nickolay Y. Gnedin,Xi Meng,Xi Meng,Vadim A. Semenov,Andrey V. Kravtsov +7 more
TL;DR: In this article, the authors present a new implementation of star formation in cosmological simulations, by considering star clusters as a unit of star creation, and they test this implementation for Milky Way-sized galaxies at high redshift, by comparing the properties of model clusters with observations of young star clusters.
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Star cluster formation in cosmological simulations. I. properties of young clusters
Hui Li,Oleg Y. Gnedin,Nickolay Y. Gnedin,Nickolay Y. Gnedin,Xi Meng,Xi Meng,Vadim A. Semenov,Andrey V. Kravtsov +7 more
TL;DR: In this article, the authors present a new implementation of star formation in cosmological simulations, by considering star clusters as a unit of star creation, and they test this implementation for Milky Way-sized galaxies at high redshift, by comparing the properties of model clusters with observations of young star clusters.
108
Gamma-rays from molecular clouds illuminated by accumulated diffusive protons. II: interacting supernova remnants
TL;DR: Li et al. as mentioned in this paper developed an accumulative diffusion model by considering an accumulation of the diffusive protons escaping from the shock front throughout the history of the SNR expansion, and applied it to nine interacting SNRs (W28, W41, W44, W49B, W51C, Cygnus Loop, IC443, CTB 37A, and G349).
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Star Cluster Formation in Cosmological Simulations. II. Effects of Star Formation Efficiency and Stellar Feedback
TL;DR: In this paper, the authors improved the algorithm by eliminating accretion gaps, boosting momentum feedback, and introducing a subgrid initial bound fraction, which distinguishes cluster mass from stellar particle mass.
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