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Table 3

Stellar parameters.

Star T eff log g V sin i v mac C/H N/H O/H
[kK] [km s-1] [km s-1] [10-4] [10-4] [10-4]

DH Cep-1 44 ± 3.0 4.3 ± 0.30 5.40* 175 100 2.3 15.0
DH Cep-2 41 ± 2.0 4.3 ± 0.20 5.50* 160 100 1.6 1.0 13.0
V382 Cyg-1 37 ± 2.0 3.8 ± 0.15 5.17 ± 0.10 260 0* 2.5 0.7 3.2
V382 Cyg-2 38 ± 3.0 3.8 ± 0.20 5.15 ± 0.14 240 0* 9.0 1.5 6.6
Y Cyg-1 33 ± 1.5 4.1 ± 0.20 4.57 ± 0.08 140 0* 1.5 0.5 3.7
Y Cyg-2 34 ± 2.0 4.2 ± 0.20 4.49 ± 0.10 160 0* 3.0 0.8 5.0
V478 Cyg-1 32 ± 2.0 3.9 ± 0.20 4.74 ± 0.11 120 0* 2.0 0.8 3.4
V478 Cyg-2 31 ± 3.0 3.7 ± 0.30 4.78 ± 0.17 120 0* 1.0 0.35 2.6
XZ Cep-1 28 ± 1.0 3.4 ± 0.15 5.05 ± 0.06 230 0* <2.0 0.6 1.0
XZ Cep-2 24 ± 3.0 3.1 ± 0.30 4.79 ± 0.22 110 0* 0.3 2.8 0.5
AH Cep-1 31 ± 3.0 4.1 ± 0.30 4.41 ± 0.17 200 0* 1.0 <0.2 2.8
AH Cep-2 29 ± 4.0 4.2 ± 0.30 4.15 ± 0.24 170 0* <2.0 0.35 2.3

Notes. A

(*)

symbol indicated adopted values from Martins et al. (2005). Luminosities are computed from Teff and Rmean (Table 4). Abundances are number ratios.

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