activity
20232026
most citedSimulating ionization feedback from young massive stars: impact of numerical resolution

16 citations · 28 across the 4 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2026

Reconstructing the Globular Cluster Initial Mass Function from Present-Day Globular Cluster Systems

Elizabeth Moreno-Hilario, Hui Li, Luis A. Martinez-Medina

The near-universal turnover mass of the present-day globular cluster mass function (GCMF), , is a well established observational featu…

astro-ph.GA2026

Identifying signatures of inflow onto face-on galaxies using the Balmer decrement

Meghna Sitaram, Hui Li, Yong Zheng +4

Isolated star-forming galaxies require inflows of fresh gas from the surrounding medium to sustain episodes of star formation over time. However, there are very few direct detectio…

astro-ph.GA20246 cited

Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping

Yuan Bian, Min Du, Victor P. Debattista +9

Most galaxies follow well-defined scaling relations of metallicity and stellar mass; however, some outliers at the low mass end of the observed galaxy population exhibit unusually…

astro-ph.GA2023

Globular Clusters Contribute to the Nuclear Star Cluster and Galaxy Center Gamma-Ray Excess, Moderated by Galaxy Assembly History

Yuan Gao, Hui Li, Xiaojia Zhang +2

Two unresolved questions at galaxy centers, namely the formation of the nuclear star cluster (NSC) and the origin of the gamma-ray excess in the Milky Way (MW) and Andromeda (M31),…

astro-ph.GA202312 cited

The influence of globular cluster evolution on the specific frequency in dwarf galaxies

Elizabeth Moreno-Hilario, Luis A. Martinez-Medina, Hui Li +2

Dwarf galaxies are known to exhibit an unusual richness in numbers of globular clusters (GCs), property quantified by the specific frequency (), which is high for dwarf and gi…

astro-ph.GA202316 cited

Simulating ionization feedback from young massive stars: impact of numerical resolution

Yunwei Deng, Hui Li, Rahul Kannan +3

Modelling galaxy formation in hydrodynamic simulations has increasingly adopted various radiative transfer methods to account for photoionization feedback from young massive stars.…