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Primordial pollution of globular clusters within their host dwarfs embedded in dark matter haloes at high redshifts
Abstract Recent observational studies have revealed star-to-star abundance inhomogeneity among light elements (e.g. C, N, O, Na and Al) of stars on the main sequence in the Galactic globular clusters (GCs). One of the promising interpretations for this result is that the observed abundance inhomogeneity is due to the second …