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收藏Figshare2019-09-29 更新2026-04-08 收录
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https://figshare.com/articles/archive_bin/9917228/1
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资源简介：
Simulation archive from REBOUND N--body simulation (see REBOUND docs for a description of simulation archives--rebound ). <br><br>We start the simulation with an eccentric disk (e=0.5) around a black hole (BH). Disk (BH) mass is 10^4 (4x10^6 Msun). Disk contains 100 stars of identical mass. GR effects are included, as is the potential due to a surrounding stellar cluster (see Madigan et al. 2009 for a model of this potential). <br>
创建时间：
2019-09-29
