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We present the abundance analysis of 97 nearby metal-poor (-3. 3-2. These results favor the scenarios that the MW thick disk formed through rapid chemical enrichment primarily through Type II supernovae of massive stars, while the stellar halo has formed at least in part via accretion of progenitor stellar systems having been chemically enriched with different timescales.
Ishigaki et al. (Thu,) studied this question.
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