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Table 6

Derived abundances for the fast rotators HD 149757 and HD 163892 for different models (spherical case vs. flattened star seen under different inclinations).

Star i [°] Abundances

C N O

(1) (2) Av.

Sph. case 7.98 7.92 8.50 8.36 8.43
HD 149757 (HARPS) 45 7.82 7.82 8.45 8.30 8.38
60 8.06 7.91 8.50 8.35 8.43
90 7.98 7.92 8.50 8.35 8.43

Sph. case 8.24 7.34 8.44 8.32 8.38
HD 163892 (FEROS) 45 8.24 7.37 8.45 8.33 8.39
60 8.24 7.37 8.45 8.33 8.39
90 8.24 7.37 8.45 8.33 8.39

Notes. (1) and (2) refer to the spectral regions 4060–4082 and 4691–4709 Å, respectively. “Av.” refers to the average of the oxygen abundances derived in the two regions.

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