Table 7
Sensitivity to the stellar flux of the different excited levels, as shown by the sum of the oscillator strengths of their lines, below or above the Balmer discontinuity (at about 3700 Å), bBD or aBD, respectively.
| E i | N bBD | ΣbBDf | N aBD | ΣaBDf | ΣbBDf/ |
| (cm-1) | ΣaBDf | ||||
|
|
|||||
| 0 | 22 | 1.3964 | 3 | 0.06763 | 20.65 |
| 416 | 29 | 1.3245 | 5 | 0.06730 | 19.68 |
| 704 | 33 | 1.3860 | 5 | 0.06491 | 21.35 |
| 888 | 29 | 1.4609 | 4 | 0.06273 | 23.29 |
| 978 | 14 | 1.5324 | 2 | 0.06410 | 23.91 |
|
|
|||||
| 6928 | 27 | 0.63980 | 3 | 0.31334 | 2.042 |
| 7377 | 34 | 0.65591 | 6 | 0.30843 | 2.127 |
| 7728 | 36 | 0.68351 | 7 | 0.29204 | 2.340 |
| 7986 | 32 | 0.65986 | 8 | 0.27952 | 2.361 |
| 8155 | 25 | 0.68376 | 6 | 0.26621 | 2.568 |
|
|
|||||
| 11 976 | 9 | 0.04452 | 8 | 0.73459 | 0.0606 |
| 12 561 | 13 | 0.04715 | 10 | 0.72093 | 0.0654 |
| 12 969 | 10 | 0.04980 | 8 | 0.73392 | 0.0679 |
Notes. NbBD and NaBD are the numbers of lines for each category, and ΣbBDf and ΣaBDf are the sums of the oscillator strengths.
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