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Table 3
Diagnostic spectral lines available in the FW model grid for late O and early-to-mid B stars in the LMC.
| Balmer series | Helium | Silicon |
|---|---|---|
| Hα | He I λ4026* | Si II λ4128 |
| Hβ | He I λ4388* | Si II λ4130 |
| Hγ* | He I λ4471* | Si II λ5041 |
| Hδ* | He I λ4713* | Si II λ5056 |
| He I λ4922* | Si III λ4553* | |
| He I λ6678* | Si III λ4568* | |
| He II λ4200* | Si III λ4575* | |
| He II λ4542* | Si III λ4813 | |
| He II λ4686* | Si III λ4820 | |
| He II λ6683 | Si III λ4829 | |
| Si IV λ4089* | ||
| Si IV λ4116* | ||
| Si IV λ4212* | ||
| Si IV λ4631 | ||
| Si IV λ4950 | ||
| Si IV λ6668 | ||
| Si IV λ6701 | ||
| Si IV λ7048 | ||
| Si IV λ8957 |
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