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Table 3
Adopted estimates for the projected rotational velocity (vesini), atmospheric parameters, silicon, magnesium and nitrogen abundance estimates.
| Star | Spectral type | vesini | Secondary | T eff | log g | v t | log ϵ + 12 | ||
| km s-1 | contribution | K | cm s-2 | km s-1 | Si | Mg | N | ||
|
|
|||||||||
| 017 | B0 V | 76 | 0% | 29 000 | 3.90 | 2 | 7.22 | 7.11 | ≤7.1 |
| 20% | 30 000 | 4.15 | 7 | 7.19 | 7.21 | ≤7.3 | |||
| 033 | B1–1.5 V | 77 | 0% | 24 000 | 3.90 | 1 | 7.21 | 7.11 | ≤6.7 |
| 20% | 23 500 | 4.15 | 6 | 7.21 | 6.95 | ≤6.8 | |||
| 179 | B1 V | 51 | 0% | 27 000 | 4.40 | 0 | 6.90 | 7.16 | ≤7.2 |
| 20% | 27 500 | 4.50 | 0 | 7.21 | 7.38 | ≤7.4 | |||
| 195 | B0.5 V | ≤40 | 0% | 28 000 | 3.90 | 0 | 7.07 | 6.86 | ≤7.1 |
| 20% | 28 000 | 4.00 | 2 | 7.23 | 7.00 | ≤7.2 | |||
| 204 | B2 III | ≤40 | 0% | 22 500 | 3.50 | 0 | 6.99 | 7.02 | ≤6.7 |
| 20% | 23 000 | 3.75 | 0 | 7.03 | 7.26 | ≤6.9 | |||
| 225 | B0.7 III–II | ≤40 | 0% | 24 500 | 3.25 | 5 | 7.22 | 7.03 | ≤7.1 |
| 20% | 25 000 | 3.45 | 8 | 7.19 | 7.16 | ≤7.3 | |||
| 299 | B0.5 V | ≤40 | 0% | 28 000 | 4.25 | 0 | 7.14 | 6.83 | ≤7.3 |
| 20% | 29 000 | 4.50 | 4 | 7.20 | 6.99 | ≤7.5 | |||
| 324 | B0.2 V | 57 | 0% | 28 500 | 3.90 | 0 | 7.19 | 7.12 | ≤7.0 |
| 20% | 30 000 | 4.25 | 5 | 7.18 | 7.23 | ≤7.1 | |||
| 351 | B0.5 V | ≤40 | 0% | 28 500 | 4.00 | 0 | 7.09 | 7.00 | ≤7.0 |
| 20% | 29 000 | 4.25 | 3 | 7.22 | 7.12 | ≤7.2 | |||
| 359 | B0.5 V | 54 | 0% | 28 000 | 4.00 | 1 | 7.17 | 7.07 | ≤7.1 |
| 20% | 29 500 | 4.40 | 6 | 7.22 | 7.18 | ≤7.2 | |||
| 534 | B0 IV | 57 | 0% | 29 000 | 3.75 | 5 | 7.20 | 6.86 | ≤7.2 |
| 20% | 29 500 | 4.00 | 9 | 7.23 | 7.08 | ≤7.2 | |||
| 575 | B0.7 III | ≤40 | 0% | 26 000 | 3.75 | 4 | 7.24 | 7.02 | 6.90 |
| 20% | 26 500 | 4.00 | 8 | 7.21 | 7.13 | 7.03 | |||
| 589 | B0.5 V | ≤40 | 0% | 27 500 | 4.00 | 0 | 6.84 | 6.75 | ≤6.9 |
| 20% | 28 500 | 4.25 | 0 | 7.14 | 6.92 | ≤7.1 | |||
| 662 | B3–5 III: | 67 | 0% | 17 500 | 3.60 | 7 | 7.16 | 6.80 | ≤7.4 |
| 20% | 18 000 | 3.90 | 11 | 7.22 | 6.94 | ≤7.5 | |||
| 665 | B0.5 V | 47 | 0% | 28 000 | 4.15 | 2 | 7.16 | 7.00 | ≤7.0 |
| 20% | 28 500 | 4.40 | 7 | 7.17 | 7.12 | ≤7.2 | |||
| 686 | B0.7 III | ≤40 | 0% | 24 000 | 3.60 | 3 | 7.16 | 6.53 | 6.65 |
| 20% | 25 000 | 3.90 | 6 | 7.20 | 6.68 | 6.76 | |||
| 723 | B0.5 V | 63 | 0% | 27 500 | 3.90 | 2 | 7.19 | 6.93 | 7.02 |
| 20% | 28 500 | 4.15 | 6 | 7.21 | 7.10 | 7.21 | |||
| 799 | B0.5–0.7 V | ≤40 | 0% | 26 500 | 4.00 | 1 | 7.15 | 6.93 | 7.33 |
| 20% | 27 000 | 4.25 | 5 | 7.17 | 7.02 | 7.45 | |||
| 850 | B1 III | ≤40 | 0% | 24 000 | 3.75 | 6 | 7.16 | 6.84 | 7.04 |
| 20% | 26 000 | 4.15 | 9 | 7.23 | 7.07 | 7.26 | |||
| 888 | B0.5 V | 76 | 0% | 27 000 | 4.15 | 0 | 7.11 | 6.97 | ≤7.0 |
| 20% | 28 500 | 4.50 | 4 | 7.22 | 7.11 | ≤7.2 | |||
Notes. For convenience the spectral types are repeated from Table 1.
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