271 citations · 2.1k across the 38 of their papers we have counts for
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Tidal disruption of stellar clusters and their remnants' spatial distribution near the galactic center
Long Wang, D. N. C. Lin
The accretion of massive star clusters via dynamical friction has previously been established to be a likely scenario for the build up of nuclear stellar clusters (NSCs). A remaini…
Dynamical Origin for the Collinder 132-Gulliver 21 Stream: A Mixture of three Co-Moving Populations with an Age Difference of 250 Myr
Xiaoying Pang, Yuqian Li, Shih-Yun Tang +6
We use Gaia DR3 data to study the Collinder 132-Gulliver 21 region via the machine learning algorithm StarGO, and find eight subgroups of stars (ASCC 32, Collinder 132 gp 1--6, Gul…
Gravitational wave of intermediate-mass black holes in Population III star clusters
Long Wang, Ataru Tanikawa, Michiko Fujii
Previous theoretical studies suggest that the Population III (Pop3) stars tend to form in extremely metal poor gas clouds with approximately embedded in mini dark ma…
Investigating the UV-excess in star clusters with -body simulations: predictions for future CSST observations
Xiaoying Pang, Qi Shu, Long Wang +1
We study the origin of the UV-excess in star clusters by performing N-body simulations of six clusters with N=10k and N=100k (single stars & binary systems) and metallicities of Z=…
SIRIUS Project. V. Formation of off-center ionized bubbles associated with Orion Nebula Cluster
Michiko S. Fujii, Kohei Hattori, Long Wang +4
Massive stars born in star clusters terminate star cluster formation by ionizing the surrounding gas. This process is considered to be prevalent in young star clusters containing m…
A tale of caution: the tails of NGC 752 are much longer than claimed
Henri M. J. Boffin, Tereza Jerabkova, Giacomo Beccari +1
Understanding the exact extent and content of tidal tails of open clusters provide useful clues on how field stars populate the Milky Way. We reanalyse, using Gaia EDR3 data, the t…