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Table 2

Estimates of the atmospheric parameters for the primaries assuming no secondary flux contribution.

Star T eff log g v t
Si λ4542 λ4686 (1) (2)

017 29 000 30 000 29 500 3.90 6 2
033   24 000 ··· ··· 3.90 3 1
179 27 000 ··· ··· 4.40 0 0
195 28 000 ··· 28 000 3.90 0 0
204   22 500 ··· ··· 3.50 0 0
225 24 500 ··· ··· 3.25 3 5
299 28 000 ··· 29 000 4.25 0 0
324 28 500 29 000 29 000 3.90 0 0
351 28 500 ··· 28 500 4.00 0 0
359 28 000 28 500 28 500 4.00 0 1
534 29 000 29 000 30 000 3.75 13 5
575 26 000 ··· 25000 3.75 0 4
589 27 500 ··· 28 000 4.00 0 0
662 17 500 ··· ··· 3.60 ··· 7
665 28 000 ··· 27 500 4.15 1 2
686 24 000 ··· ··· 3.60 4 3
723 27 500 ··· 27 000 3.90 0 2
799 26 500 ··· 26 000 4.00 2 1
850 24 000 ··· ··· 3.75 22 6
888 27 000 ··· 27 000 4.15 6 0

Notes. Effective-temperature estimates are from the silicon ionisation balance (Si) or the He ii profiles at 4541 and 4686 Å. The former used the microturbulent velocity estimates from the absolute silicon abundance (method 2). Microturbulence estimates are from the relative strengths of the Si iii triplet (1) or the absolute silicon abundance (2).

(†)

Teff estimates from absence of Si ii and Si iv lines.

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