- 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
determined with TURBOSPECTRUM from the 3D
and 1D models, except for O and Li, where a full 3D analysis was performed
and we give two values: the abundance correction 3D - 3D
(``3D'') and ``1D'' = 3D - 1D
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.
are the abundance changes caused
by changes in
of 100 K (A) or 150 K (B), in
0.1 dex, and by 0.5
in the microturbulence velocity .
Other column headings and comments as in Table 3.
- Table 5:
Li abundances in CS 22876-032.
corrections for depletion by diffusion (see text).
- Table 6:
3D abundance corrections for the OH lines. [O/H] and [O/Fe] are relative to
- Table 7:
1D gravity effects on the Fe and O abundances.
- Table 1:
Radial-velocity observations of CS 22876-032. For each
is the estimated error and (O-C) the residual
from the orbital fit. : H velocities; omitted from
- 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.