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Table 2
Si lines used to determine the effective temperature in B stars.
| Si II | Si III | Si IV |
|
|
||
| 4128.054 |
4567.840 |
4212.405 |
| 4130.894 |
4574.757 |
6701.12 |
| 5056.150 |
4813.33 | |
| 6371.371 |
4829.073 | |
| 5716.287 | ||
| 5739.734 |
||
Notes. Lines present in the spectrum of HD 48977 are underlined. Lines that should be avoided according to Simón-Díaz (2010) are listed in italics.
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