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Table 4
Nitrogen abundance estimates and projected rotational velocities for targets for which a reliable effective-temperature estimate could not be obtained.
| Star | ST | vesini | log g | log ϵN + 12 |
| km s-1 | cm s-2 | |||
|
|
||||
| 018 | B1.5 V | 48 | 3.70 | ≤7.5 |
| 041 | B2: V | ≤40 | 3.90 | ≤7.6 |
| 162 | B0.7 V | 60 | 4.10 | ≤7.3 |
| 218 | B1.5 V | 79 | 3.75 | ≤6.9 |
| 342 | B1 V | ≤40 | 4.05 | 6.86–7.11 |
| 434 | B1.5: V | 45 | 3.95 | 7.00–7.26 |
| 501 | B0.5 V | 59 | 4.00 | 6.55–6.71 |
| 520 | B1: V | 53 | 4.10 | ≤7.3 |
| 719 | B1 V | 50 | 3.95 | ≤7.2 |
| 742 | B2 V | 60 | 4.05 | ≤7.4 |
| 792 | B2 V | 47 | 4.05 | 6.98–7.20 |
| 874 | B1.5 IIIe+ | 62 | 3.55 | 6.67–6.81 |
| 891 | B2 V | 55 | 4.00 | ≤7.3 |
Notes. The gravity estimate is for Teff = 23 000 K and a zero microturbulence has been adopted. For convenience the spectral types (ST) are repeated from Table 1.
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