Data: Dynamics of star clusters with tangentially anisotropic velocity distribution (Pavlik+ 2024)

This dataset represents the results of our N-body simulations of star clusters (SCs). The initial conditions of the models are fully described in the referenced journal article. In short, the SCs start from isotropic, radially anisotropic or tangentially anisotropic initial velocity distributions, and each model is evolved in an external Galactic tidal field, for two different choices of the filling factor.

Pavlík, V., Heggie, D. C., Varri, A. L., & Vesperini, E. (2024). Data: Dynamics of star clusters with tangentially anisotropic velocity distribution (Pavlik+ 2024) [Data set]. In Astronomy & Astrophysics (Vol. 689, p. A313). Zenodo. https://doi.org/10.5281/zenodo.12759107