Globular Clusters in a Cosmological N-body Simulation
Stellar dynamical model globular clusters are introduced into reconstituted versions of the dark matter halos of the Via Lactea II (VL-2) simulation to follow the star cluster tidal mass-loss and stellar stream formation. The clusters initially evolve within their local sub-galactic halo, later bein...
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Published in | The Astrophysical journal Vol. 861; no. 1; pp. 69 - 80 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
Philadelphia
The American Astronomical Society
01.07.2018
IOP Publishing |
Subjects | |
Online Access | Get full text |
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