Subvirial Simulations
收藏DataCite Commons2024-09-15 更新2024-07-13 收录
下载链接：
https://orda.shef.ac.uk/articles/dataset/Subvirial_Simulations/25205207/1
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资源简介：
20 subvirial simulations of 1000 stars with an initial fractal dimension of 1.6, meaning the initial distribution of stars is clumpy.
Originally used in Blaylock-Squibbs & Parker (2024) 'The dynamical evolution of star-forming regions measured with INDICATE'.
The simulations are run using the <em>kira</em> integrator which is part of <em>starlab</em>: https://www.sns.ias.edu/~starlab/index.html
The simulations are purely dynamical with no stellar evolution. We do not simulate the gas potential the stars would be embedded in, nor do we simulate the galactic tidal field. The simulations show 10 Myr of purely dynamic evolution.
提供机构：
The University of Sheffield
创建时间：
2024-02-13
