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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Bibliographic Details
Published inThe Astrophysical journal Vol. 861; no. 1; pp. 69 - 80
Main Author Carlberg, Raymond G.
Format Journal Article
LanguageEnglish
Published Philadelphia The American Astronomical Society 01.07.2018
IOP Publishing
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