Centrally concentrated star formation in young clusters
This repository provides visualizations for all simulations presented in the manuscript. For each model and output snapshot, we include ProjectPlots (line-of-sight projections) and SlicePlots (mid-plane sections). All plots were generated with the yt analysis toolkit from the simulation outputs and finalized using Matplotlib. Spatial scales, physical units, and color normalization are standardized within each run, enabling quantitative and directly comparable analyses of morphology and temporal evolution. Stellar positions are overplotted: black dots denote all stars, while red dots indicate stars with masses greater than 15 MSun. These visualizations accompany the article submitted to Astronomy & Astrophysics on the early dynamical evolution of embedded star clusters (Adilkhan et al. 2025).
Institutions
- American Museum of Natural History (US)
- Al-Farabi Kazakh National University (KZ)
- Fesenkov Astrophysical Institute (KZ)
- Simons Foundation (US)
- Max Planck Institute for Astronomy (DE)
- Nazarbayev University (KZ)
- Drexel University (US)
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2025-08-30
- DOI
- https://doi.org/10.5281/zenodo.17005409
- Primary Topic
- Geochemistry and Geologic Mapping
- Type
- article
- Field-Weighted Citation Impact
- 0.00