On the origin of the stellar halo and multiple stellar populations in the globular cluster NGC 1851
We propose that the observed stellar halo around the globular cluster (GC) NGC 1851 is evidence of its formation in the central region of its defunct host dwarf galaxy. We numerically investigate the long-term dynamical evolution of a nucleated dwarf galaxy embedded in a massive dark matter halo under the strong tidal field of the Galaxy. The dwarf galaxy is assumed to have a stellar nucleus (or a nuclear star cluster) that could be the progenitor for NGC 1851. We find that although the dark...[Show more]
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|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Bekki_On_the_origin_of_the_stellar_2012.pdf||1.98 MB||Adobe PDF||Request a copy|
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