Galactic evolution of oxygen - OH lines in 3D hydrodynamical model atmospheres

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Table 5:

1D Fe abundances for six stars in the sample of Israelian et al. (1998,2001), from three Fe I lines of different excitation potentials.
Star	$T_{\rm eff}\;$	$\log{g}\;$	$\xi_t$	[Fe/H]	[Fe I/H]₃₁₄₃	[Fe I/H]₃₁₄₉	[Fe I/H]₃₁₅₂
	[K]	[dex]	[ ${\rm km}\:{\rm s}^{-1}\;$ ]	[dex]	[dex]	[dex]	[dex]
G 64-12	6318	4.20	1.0	-3.37	-3.44	-3.38	-3.43
G 64-37	6310	4.20	1.0	-3.22	-3.22	-3.21	-3.19
LP 815-43	6265	4.54	1.0	-3.05	-3.06	-2.92	-3.05
HD 140283	5550	3.35	1.0	-2.70	-2.77	-2.57	-2.83
HD 166913	5965	3.90	1.0	-1.80	-	-1.57	-1.78
HD 76932	5800	3.85	1.0	-1.10	-	-1.48	-1.45

Source LaTeX | All tables | In the text

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