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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 10.

Overview of the merger system at 160 Myr simulation time. The result is obtained with the SDT model. The background gray-scale map is the gas surface density projected along the x-axis, while the colorful dots with different sizes are the young stars (age <5 Myr) with different masses.

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