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The Star Clusters as Links between Galaxy Evolution and Star Formation Project. I. Numerical Method

  • Authors: Marta Reina-Campos, Oleg Y. Gnedin, Alison Sills, Hui Li

Marta Reina-Campos et al 2025 The Astrophysical Journal 978 .

  • Provider: AAS Journals

Caption: Figure 3.

Time evolution of the projected gas surface density (top row) and the projected ionized gas surface density (bottom row) of the fiducial cloud at three representative times (0.5t ff, t ff, and 1.5t ff). The star clusters are represented by red markers, scaled by mass. The black markers indicate sinks without stellar populations, i.e., representing dense clumps of gas.

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