Impact of NLTE on determinations of atmospheric parameters and chemical abundances of very metal-poor stars
classification
🌌 astro-ph.SR
keywords
abundanceschemicalmetal-poorstarsveryatmosphericavailablecomputational
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Based on high-resolution spectral observations for a sample of very metal-poor stars, we investigate how well stellar chemical abundances can be derived with available theoretical methods and computational tools.
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