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Table 4
Elemental abundances (log NX/Ntot) compared to the sun’s abundances.
| Element | Component A | Component B | Sun |
|
|
|||
| Fe | −4.85 (0.3;28) | −4.44 (0.2;28) | −4.54 |
| Ca | −5.67 (0.18;8) | −5.70 (0.27;6) | −5.70 |
| Ni | −5.82 (0.19;5) | −5.44 (0.16;6) | −5.82 |
| Mg | −4.43 (0.08;3) | −4.70 (0.30;4) | −4.44 |
| Ti | −7.60 (0.37;3) | −7.40 (0.55;3) | −7.09 |
| Ba | −8.76 (0.33;3) | −8.90 (0.13;3) | −9.86 |
| Y | −9.33 (0.36;3) | −8.98 (0.54;2) | −9.83 |
| Sc | −9.10 (−;1) | −10.05 (0.25;3) | −8.89 |
| Si | −4.60 (0.16;3) | −4.35 (0.23;2) | −4.53 |
| S | −4.73 (0.01;2) | −4.85 (0.07;2) | −4.92 |
| Mn | −7.00 (0.14;2) | −6.61 (−;1) | −6.61 |
| O | −3.27 (−;1) | −3.35 (−;1) | −3.35 |
| C | −4.11 (−;1) | −3.85 (−;1) | −3.61 |
| Li | −9.50 (−;1) | −9.50 (−;1) | −10.99 |
|
|
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| La | −9.94 (−;1) | −9.94 (−;1) | −10.94 |
| Ce | −9.46 (−;1) | −9.46 (−;1) | −10.46 |
| Sr | −8.67 (−;1) | −8.17 (−;1) | −9.17 |
| Zr | −8.46 (−;1) | −8.96 (−;1) | −9.46 |
| Nd | −10.62 (−;1) | −9.62 (−;1) | −10.62 |
| Eu | −10.52 (−;1) | −10.52 (−;1) | −11.52 |
| Lu | −11.0 (−;1) | −10.44 (−;1) | −11.94 |
Notes. The first number in brackets is the standard deviation and the numbers of lines are separated by “;”. The solar abundances are taken from Asplund et al. (2009). The abundances of the elements below the line are derived by fitting line blends.
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