X. Pang

activity

20242026

most citedRapid formation of a very massive star >50000

M_{⊙}

and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters

16 citations · 37 across the 9 of their papers we have counts for

collaborators

Showing 2024Show all

2 papers · 1 filter

astro-ph.GA2024★ 3 cited

The 3D morphology of open clusters in the solar neighborhood III: Fractal dimension

Chang Qin, Xiaoying Pang, Mario Pasquato +2

We analyze the fractal dimension of open clusters using 3D spatial data from Gaia DR3 for 93 open clusters from Pang et al. (2024) and 127 open clusters from Hunt & Reffert (2024)…

astro-ph.GA2024★ 5 cited

Cluster membership analysis with supervised learning and $N$ -body simulations

A. Bissekenov, M. Kalambay, E. Abdikamalov +3

Membership analysis is an important tool for studying star clusters. There are various approaches to membership determination, including supervised and unsupervised machine learnin…

The 3D morphology of open clusters in the solar neighborhood III: Fractal dimension

Cluster membership analysis with supervised learning and N-body simulations

Cluster membership analysis with supervised learning and $N$ -body simulations