A differential study of the oxygen abundances in the Galactic thin and thick disks

First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented. Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim 215000$) and high signal-to-noise ($S\mathrm{/}N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined. Our findings can be summarized as follows: {\bf 1)} at $[\mathrm{F}\mathrm{e}\mathrm{/}\mathrm{H}]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $[\mathrm{O}\mathrm{/}\mathrm{F}\mathrm{e}]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $[\mathrm{F}\mathrm{e}\mathrm{/}\mathrm{H}]\sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $[\mathrm{O}\mathrm{/}\mathrm{F}\mathrm{e}]$ continues to decrease at $[\mathrm{F}\mathrm{e}\mathrm{/}\mathrm{H}]>0$ without showing the leveling out that previously has been seen.