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[ascl:2212.019] m2mcluster: Star clusters made-to-measure modeling

m2mcluster performs made-to-measure modeling of star clusters, and can fit target observations of a Galactic globular cluster's 3D density profile and individual kinematic properties, including proper motion velocity dispersion, and line of sight velocity dispersion. The code uses AMUSE (ascl:1107.007) to model the gravitational N-body evolution of the system between time steps; GalPy (ascl:1411.008) is also required.

Code site:
https://github.com/webbjj/m2mcluster
Described in:
https://ui.adsabs.harvard.edu/abs/2022arXiv221206847W
Bibcode:
2022ascl.soft12019W

Views: 889

ascl:2212.019
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