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Table 6

Comparison of nitrogen abundances from tlusty and fastwind analyses.

Star Spectral type tlusty fastwind
T eff log g v t N T eff log g He N

028 B0.7 Ia Nwk 24 000 2.75 14 7.32 24 000 2.75 0.10 7.36
069 B0.7 Ib-Iab 23 500 2.75 15 7.93 24 000 2.75 0.10 7.93
082 B0.5 Ib-Iab 25 500 3.00 13 7.89 26 500 3.00 0.15 8.10
087 O9.7 Ib-II 29 000 3.25 12 7.29 30 000 3.20 0.10 7.80
165 O9.7 Iab 27 000 3.00 14 7.86 28 000 3.00 0.15 8.16
270 B3 Ib 17 500 2.90 1 7.57 17 500 2.90 0.10 7.57
431 B1.5 Ia Nstr 19 000 2.35 18 7.98 19 000 2.40 0.10 8.10
578 B1.5 Ia Nwk 21 500 2.75 11 7.07 21 500 2.75 0.10 6.96
831 B5 Ia 14 000 2.10 21 8.02 13 000 1.85 0.10 8.22
845 B1 II 23 500 3.25 7 7.54 23 500 3.25 0.10 7.54
867 B1 Ib Nwk 24 500 3.15 11 7.16 26 000 3.25 0.08 7.16

Notes. The former are taken from Table 4, and the tlusty microturbulences were used for the fastwind analysis. Abundances are presented on the scale log(X/H) + 12.

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