Potential impact of the Sagittarius dwarf galaxy on the formation of young O-rich stars.

Nat Commun · 2025 · PMC11822012 · PMID 39939596

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an increasing trendno p-value reported

Figure 3 a, b, d, e shows that there is an increasing trend of [O/Fe] with decreasing age in young (age < 3 Gyr) and intermediate (4 Gyr < age < 6 Gyr) populations.

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