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Table 3

Atmospheric parameters and metal abundances derived in this work for the slow rotators.

Star T eff [K] log g log ϵ(C)4060–4082 Å log ϵ(N)4995–5011 Å log ϵ(O)
y
[N/C] [N/O]
4060–4082 Å 4691–4709 Å Adopted

ξ1 CMa 28 200 3.90 0.105 7.90 7.84 8.40 8.54 8.47 –0.06 –0.63
28 500 4.00 0.112 8.10 7.80 8.46 8.60 8.53 –0.30 –0.73

τ Sco 31 200 4.30 0.083 8.18 7.90 8.27 8.50 8.39 –0.28 –0.49
31 000 4.40 0.083 8.40 7.90 8.24 8.62 8.43 –0.50 –0.53

HD 57682 33 400 4.00 0.082 8.06 7.60 8.24 8.26 8.25 –0.46 –0.65
33 300 4.00 0.083 7.98 7.76 8.42 8.30 8.36 –0.22 –0.60

10 Lac 34 300 4.20 0.077 8.22 7.42 8.34 8.28 8.31 –0.80 –0.89
34 000 4.20 0.072 8.20 7.80 8.48 8.24 8.36 –0.40 –0.56

Typical errors 1000 0.10 0.025 0.12 0.13 ... ... 0.21 0.21 0.12

Notes. For each star, the first row gives our nominal results, while the second row (in italics) provides the results obtained with spectra convolved with v sin i= 300 km s-1. Note that solar [N/C] and [N/O] abundance ratios are –0.60 and –0.86, respectively (Asplund et al. 2009).

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