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Table 3
Derived abundances from individual lines of Si ii for a selection of stars in our sample.
| HgMn stars | Normal stars | Magnetic stars | |||||||||||||
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| HD | HD | HD | |||||||||||||
| Line (Å) | 178 065 | 27 295 | 57 608 | 78 316 | 222 173 | 22 136 | 170 054 | 162 586 | 74 168 | 49 333 | 223 640 | 47 116 | |||
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| 4621 | −4.67 | −4.52 | −4.89 | −4.34 | −4.66 | −4.67 | −4.64 | −4.67 | −4.00 | −3.90 | −3.09 | −3.21 | |||
| 5041−55−56 | −4.56 | −4.58 | −4.78 | −4.44 | −4.63 | −4.64 | −4.81 | −4.82 | −4.11 | −4.15 | −3.20 | −3.48 | |||
| 5957−78 | – | −4.54 | −4.66 | −4.26 | −4.48 | −4.59 | −4.70 | −4.72 | −3.93 | −3.91 | −2.98 | −3.27 | |||
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| Dispersion | – | 0.03 | 0.12 | 0.09 | 0.10 | 0.04 | 0.09 | 0.08 | 0.09 | 0.14 | 0.11 | 0.14 | |||
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