Oxygen In The Galactic Disk: Non-LTE Abundances From The 777 nm O I Triplet
Oxygen abundances for a large sample of dwarf stars in the Galactic thin and thick disks are determined from a non-LTE analysis of the oxygen triplet lines at 777 nm. Kinematic criteria are employed to determine whether a star belongs to the thin or thick disk. Temperatures are obtained from photometric calibrations based on the infrared flux
Ramirez, I. et al.
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2004