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20112024
most citedA catalog of newly identified star clusters in GAIA DR2

233 citations · 811 across the 26 of their papers we have counts for

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Showing 2022Show all

5 papers · 1 filter

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★ 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=…

astro-ph.GA2022★ 15 cited

Searching for multiple populations in star clusters using the China Space Station Telescope

Chengyuan Li, Zhenya Zheng, Xiaodong Li +6

Multiple stellar populations (MPs) in most star clusters older than 2 Gyr, as seen by lots of spectroscopic and photometric studies, have led to a significant challenge to the trad…

astro-ph.GA2022★ 37 cited

The impact of stellar evolution on rotating star clusters: the gravothermal-gravogyro catastrophe and the formation of a bar of black holes

A. W. H. Kamlah, R. Spurzem, P. Berczik +7

We present results from a suite of eight direct N-body simulations, performed with \textsc{Nbody6++GPU}, representing realistic models of rotating star clusters with up to $1.1\tim…

astro-ph.GA2022★ 57 cited

3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR3 II: Hierarchical Star Formation Revealed by Spatial and Kinematic Substructures

Xiaoying Pang, Shih-Yun Tang, Yuqian Li +9

We identify members of 65 open clusters in the solar neighborhood using the machine-learning algorithm StarGO based on Gaia EDR3 data. After adding members of twenty clusters from…