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Individual Star Sampling in Star Formation Simulations: A Semideterministic Model

  • Authors: Yunwei Deng, 云未 邓, Hui Li, 辉 李, Zhiqiang Yan, 智强 闫, Chuizheng Kong, 垂政 孔, Zhi-Yu Zhang, 智昱 张

Yunwei Deng et al 2026 The Astrophysical Journal Supplement Series 286 .

  • Provider: AAS Journals

Caption: Figure 12.

Most-massive stellar mass to embedded cluster mass (m⋆,max–Mecl) relation in the simulations. The clusters are identified by the 4D FoF method. Blue, green, and red curves are the median results for simulations using RND, NGB, and SDT methods, respectively. The shaded regions are the 16th–84th percentile ranges. Gray crosses are the observational data.

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