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

Name: Data: Dynamics of star clusters with tangentially anisotropic velocity distribution (Pavlik+ 2024)
Creator: Indiana University Bloomington, Department of Astronomy; School of Mathematics and Maxwell Institute for Mathematical Sciences, University of Edinburgh; Institute for Astronomy, University of Edinburgh, Royal Observatory; Czech Academy of Sciences, Astronomical Institute
Published: 2024-09-20T00:00:00+08:00

Zenodo2024-09-20 更新2026-04-07 收录

星团动力学模拟

N体数值模拟

数据链接：

https://zenodo.org/doi/10.5281/zenodo.12759107 数据链接链接失效反馈

官方服务：

资源简介：

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.

提供机构：

Indiana University Bloomington, Department of Astronomy; School of Mathematics and Maxwell Institute for Mathematical Sciences, University of Edinburgh; Institute for Astronomy, University of Edinburgh, Royal Observatory; Czech Academy of Sciences, Astronomical Institute

创建时间：

2024-09-20