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Table 1

Lithium abundance vs. changes of input parameters.

log NLTE(Li) Star Teff (K) logg Vm (km s−1)
–50 +50 –0.2 +0.2 –0.2 +0.2
0.98 HD 220981 +0.05 (5) –0.05 (5) 0.0 (5) 0.0 (5) 0.0 (5) 0.0 (5)
1.00 HIP 66990 +0.05 (4) –0.05 (4) 0.0 (4) 0.0 (4) 0.0 (4) 0.0 (4)
1.02 HD 49866 +0.05 (4) –0.05 (4) 0.0 (4) 0.0 (4) 0.0 (4) 0.05 (5)
1.48 HD 221954 +0.05 (4) –0.05 (4) 0.0 (4) 0.0 (4) 0.0 (4) 0.0 (5)
1.50 HD 193995 +0.05 (5) –0.05 (5) 0.0 (5) 0.0 (5) 0.0 (4) 0.0 (5)
1.54 HD 7950 +0.05 (4) –0.05 (4) 0.0 (4) 0.0 (4) 0.0 (4) 0.0 (4)
1.90 HD 78130 0.00 (4) –0.05 (5) 0.0 (5) 0.0 (5) 0.0 (5) 0.0 (5)
1.96 HD 19493 +0.05 (4) –0.05 (3) 0.0 (4) 0.0 (4) 0.0 (3) 0.0 (4)
2.17 HD 56957 +0.05 (5) –0.05 (5) 0.0 (5) 0.0 (5) 0.0 (5) 0.0 (5)
2.43 HD 101348 +0.05 (6) –0.05 (5) 0.0 (5) 0.0 (5) 0.0 (5) 0.0 (6)
2.48 HD 6790 +0.04 (6) –0.01 (6) +0.01 (6) +0.01 (6) 0.01 (6) 0.01 (6)
2.55 HD 90520 0.0 (5) –0.01 (6) 0.0 (6) 0.0 (6) 0.0 (6) 0.0 (6)
2.75 HD 10188 +0.05 (5) 0.0 (5) 0.0 (6) 0.0 (5) 0.0 (5) 0.0 (5)
2.90 HD 19773 0 (5) –0.05 (5) –0.05 (4) 0.0 (5) –0.05 (4) 0.0 (5)
3.01 HD 189627 0.05 (9) –0.05 (9) 0.0 (9) 0.0 (9) 0.0 (9) 0.0 (9)

Notes. Numbers in brackets show the V sin i used to adjust the fit of the synthetic spectra to the resonance lithium doublet profile (see Ivanyuk et al. 2017).

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