A dwarf-dwarf merger and dark matter core as a solution to the globular cluster problems in the Fornax dSph
The five globular clusters (GCs) of the Fornax dwarf spheroidal galaxy are puzzling for two reasons; the mass in GCs is high with respect to the galaxy's old stellar mass and their survival and large distance (>1 kpc) is at odds with naive expectations of dynamical friction. We present here a semi-analytic model, simultaneously addressing both
Leung, Gigi Y. C. et al.
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2020