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Table 3
Equivalent widths for the available metallic lines of the secondary.
| Species | λ (Å) | EWmeas. (mÅ) | EWcorr. (mÅ) | [X/H] |
|
|
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| N II | 3995 | 62 | 98 | 7.54 |
| O II | 4069 | 89 | 129 | 8.19 |
| O II | 4072 | 65 | 99 | 8.34 |
| O II | 4076 | 75 | 117 | 8.35 |
| O II | 4591 | 51 | 80 | 8.21 |
| O II | 4596 | 48 | 75 | 8.23 |
| O II | 4662 | 42 | 66 | 8.04 |
| Mg II | 4481 | 53 | 34 | 6.68 |
| Si III | 4553 | 87 | 142 | 6.88 |
| Si III | 4568 | 69 | 108 | 6.85 |
| Si III | 4575 | 42 | 66 | 6.90 |
| Si IV | 4116 | 25 | 39 | 6.85 |
Notes. Abundances (where [X/H] = log(X/H) + 12) have been calculated by scaling the measured equivalent widths (EWmeas.) to give corrected widths (EWcorr.) assuming that the secondary is 1.8 times brighter than the primary.
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