Understanding the chemical evolution of C, O, N, Ne, S, Cl and Ar in the Milky Way using H II regions
We use a sample of 33 H II regions with high and intermediate resolution spectroscopy to analyze the radial distribution of different elements in the Milky Way. This sample covers Galactocentric distances from 6 to 17 kpc, which have been revised using Gaia DR2 parallaxes. We calculate physical conditions and chemical abundances using updated
Arellano-Córdova, K. Z. et al.
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2020