Table 2
LTE atmospheric abundances of HD 45975 derived using the two independent analyses.
| HD 45975 | Sun | ||||
|
|
|||||
| First analysis | Second analysis | ||||
|
|
|||||
| Element |
|
n |
|
n |
|
|
|
|||||
| He | −1.40 ± 0.23 | 2 | −1.11 | ||
| C | −3.77 ± 0.32 | 1 | −3.78 ± 0.32 | 1 | −3.61 |
| O | −3.35 ± 0.22 | 4 | −3.47 ± 0.09 | 2 | −3.35 |
| Mg | −4.93 ± 0.20 | 10 | −4.74 ± 0.17 | 4 | −4.44 |
| Al | −6.55 ± 0.05 | 2 | −6.40 ± 0.21 | 1 | −5.59 |
| Si | −4.75 ± 0.21 | 16 | −4.87 ± 0.17 | 4 | −4.53 |
| S | −5.13 ± 0.34 | 7 | −4.75 ± 0.20 | 4 | −4.92 |
| Ca | −5.76 ± 0.29 | 1 | −5.61 ± 0.29 | 1 | −5.70 |
| Sc | −9.07 ± 0.29 | 1 | −8.89 | ||
| Ti | −5.87 ± 0.26 | 26 | −5.88 ± 0.24 | 35 | −7.09 |
| Cr | −5.65 ± 0.26 | 29 | −5.44 ± 0.18 | 36 | −6.40 |
| Mn | −4.60 ± 0.28 | 73 | −4.37 ± 0.22 | 63 | −6.61 |
| Mn (HFS) | −4.55 ± 0.12 | 4 | −6.61 | ||
| Fe | −4.86 ± 0.18 | 65 | −4.80 ± 0.17 | 46 | −4.54 |
| Ni | −6.82 ± 0.18 | 4 | −5.82 | ||
| Gaa | −5.94 ± 0.27 | 1 | −9.00 | ||
| Ga (HFS)a | −5.30 ± 0.27 | 1 | −9.00 | ||
| Sr | −8.83 ± 0.35 | 1 | −9.76 ± 0.35 | 1 | −9.17 |
| Y | −6.33 ± 0.27 | 17 | −6.51 ± 0.23 | 19 | −9.83 |
| Hg | −5.36 ± 0.38 | 4 | −4.87 ± 0.17 | 4 | −10.87 |
Notes. 
is the number density of the species and n is the number of
measured lines. The Mn and Ga abundances are given taking into account or ignoring
HFS effects. For comparison purposes, the last column lists the (rescaled) solar
abundances derived from 3D hydrodynamical model atmospheres (Asplund et al. 2009).
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