
doi: 10.5281/zenodo.5076036 , 10.5281/zenodo.6639056 , 10.5281/zenodo.4719839 , 10.5281/zenodo.3260650 , 10.5281/zenodo.7347303 , 10.5281/zenodo.4686872 , 10.5281/zenodo.3885168 , 10.5281/zenodo.3520561 , 10.5281/zenodo.4575510 , 10.5281/zenodo.7799235 , 10.5281/zenodo.5075419 , 10.5281/zenodo.7687785 , 10.5281/zenodo.8409512 , 10.5281/zenodo.1443252 , 10.5281/zenodo.4531372 , 10.5281/zenodo.7944841 , 10.5281/zenodo.3520543 , 10.5281/zenodo.6325523 , 10.5281/zenodo.4946130 , 10.5281/zenodo.3663633 , 10.5281/zenodo.3531885 , 10.5281/zenodo.3553803 , 10.5281/zenodo.7944359 , 10.5281/zenodo.4719906 , 10.5281/zenodo.3466805 , 10.5281/zenodo.4720106 , 10.5281/zenodo.4573795 , 10.5281/zenodo.3524896 , 10.5281/zenodo.7684709 , 10.5281/zenodo.1435860 , 10.5281/zenodo.7180918
doi: 10.5281/zenodo.5076036 , 10.5281/zenodo.6639056 , 10.5281/zenodo.4719839 , 10.5281/zenodo.3260650 , 10.5281/zenodo.7347303 , 10.5281/zenodo.4686872 , 10.5281/zenodo.3885168 , 10.5281/zenodo.3520561 , 10.5281/zenodo.4575510 , 10.5281/zenodo.7799235 , 10.5281/zenodo.5075419 , 10.5281/zenodo.7687785 , 10.5281/zenodo.8409512 , 10.5281/zenodo.1443252 , 10.5281/zenodo.4531372 , 10.5281/zenodo.7944841 , 10.5281/zenodo.3520543 , 10.5281/zenodo.6325523 , 10.5281/zenodo.4946130 , 10.5281/zenodo.3663633 , 10.5281/zenodo.3531885 , 10.5281/zenodo.3553803 , 10.5281/zenodo.7944359 , 10.5281/zenodo.4719906 , 10.5281/zenodo.3466805 , 10.5281/zenodo.4720106 , 10.5281/zenodo.4573795 , 10.5281/zenodo.3524896 , 10.5281/zenodo.7684709 , 10.5281/zenodo.1435860 , 10.5281/zenodo.7180918
A Python framework to combine existing astrophysical simulation codes in numerical experiments. With AMUSE you can simulate objects such as star clusters, proto-planetary disks and galaxies.
astronomy, model coupling, multi-model simulation, physics
astronomy, model coupling, multi-model simulation, physics
| 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). | 9 | |
| 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. | Top 10% | |
| 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 |
