All Tables

Table 2: Orbital elements of CS 22876-032.
Table 3: Element abundances of CS 22876-032. The Solar O abundance is adopted from the 3D measurement of atomic lines of Ludwig & Steffen (2007); the other Solar abundances from Grevesse & Sauval (2000). [X/H] and [X/Fe] are LTE values; [X/Fe] refers to Fe I for OH and neutral species, to Fe II for ionised species. The 3D abundance corrections $\Delta _{\rm 3D-1D}$ were determined with TURBOSPECTRUM from the $\langle$ 3D $\rangle$ and 1D models, except for O and Li, where a full 3D analysis was performed and we give two values: the abundance correction 3D - $\langle$ 3D $\rangle$ (`` $\langle$ 3D $\rangle$ '') and ``1D'' = 3D - 1D $_{\rm LHD}$ (see text). $\sigma$ is the standard deviation of the results from the n lines (next column; if n=1, the wavelength of the line in nm is given). See text for details on the measurement of Li, O, Sc, and Co.
Table 4: Abundance errors in CS 22876-032. $\Delta _{T_{\rm eff}}$ , $\Delta_{\log g}$ , and $\Delta _{\xi }$ are the abundance changes caused by changes in $T_{\rm eff}$ of 100 K (A) or 150 K (B), in $\log g$ by 0.1 dex, and by 0.5 ${\rm km}\:{\rm s}^{-1}\;$ in the microturbulence velocity $\xi$ . Other column headings and comments as in Table 3.
Table 5: Li abundances in CS 22876-032. $A{\rm (Li)_{1D,NLTE,DC}}$ includes corrections for depletion by diffusion (see text).
Table 6: 3D abundance corrections for the OH lines. [O/H] and [O/Fe] are relative to $\log \epsilon({\rm O})_{\odot}=8.72$ .
Table 7: 1D gravity effects on the Fe and O abundances.
Table 1: Radial-velocity observations of CS 22876-032. For each velocity, $\sigma$ is the estimated error and (O-C) the residual from the orbital fit. $^\star$ : H $_\alpha$ velocities; omitted from solution.
Table A.1: Line data, equivalent widths, veiling factors and 1D abundances of CS 22876-032A, B.
Table A.2: Hyperfine structure of Sc and Co.