40 citations · 54 across the 4 of their papers we have counts for
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astro-ph.GA2022★ 6 cited
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…
astro-ph.GA2022★ 40 cited
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…
astro-ph.GA2022★ 6 cited
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=…