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Table 5

Effects of 20% secondary contribution.

Star Secondary T eff log g v t Mg  N estimates
contribution λ3995 all lines

687 0% 20 000 2.65 18 7.00 6.94 7.00
20% 20 500 2.75 26 7.08 7.02 7.17

675 0% 22 500 2.75 12 7.08 6.93 7.10
20% 24 000 3.15 20 7.11 7.00 7.20

672 0% 25 000 3.00 10 7.04 6.85
20% 27 000 3.60 18 7.07 6.90

Notes. Abundances are presented on the scale log(X/H) + 12.

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