
** this file is automatically downloaded by Phantom when running the starcluster setup ** This is a small ascii file containing positions and velocities of stars utilised in the "starcluster" configuration in the Phantom smoothed particle hydrodynamics and magnetohydrodynamics code (Price et al. 2018). It is used to set up a collection of N-body particles. The star cluster setup (and the data file) were written by Yann Bernard as part of his PhD thesis at Université Grenoble Alpes. The datafile is published here so it can be used in the automated code testing via github actions. The columns are mass, position (x,y,z) and velocity (vx,vy,vz) for all of the stars in the simulation
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
