Young stars across Orion's four groups share sub-solar carbon, magnesium, silicon, potassium, titanium, and iron abundances, with a lower alpha-to-iron ratio than nearby older stars.
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Atmospheric parameters and chemical abundances of young stars with APOGEE. I. Orion star-forming region
Young stars across Orion's four groups share sub-solar carbon, magnesium, silicon, potassium, titanium, and iron abundances, with a lower alpha-to-iron ratio than nearby older stars.