1/1
Supervirial Simulations
dataset
posted on 2024-02-13, 08:27 authored by George Blaylock-SquibbsGeorge Blaylock-Squibbs, Richard ParkerRichard Parker20 supervirial (region is expanding) 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 kira integrator which is part of starlab: 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.
History
Ethics
- There is no personal data or any that requires ethical approval
Policy
- The data complies with the institution and funders' policies on access and sharing
Sharing and access restrictions
- The uploaded data can be shared openly
Data description
- The file formats are open or commonly used
Methodology, headings and units
- There is a file including methodology, headings and units, such as a readme.txt
