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Table 2

Fundamental stellar parameters which are used when generating model atmospheres for our stars.

Name Teffa log g b log g [Fe/H]b ξ micro c ξ micro d ξmicro ξmacro [α/ Fe]e
[K] (cgs) (cgs) [km s-1] [km s-1] [km s-1] [km s-1]
PARAM 1.1 Gaia-ESO Tsuji (85, 08) final FWHM

β Peg 3448 ± 42 0.54 0.19 ± 0.11 −0.11 f 1.7 ± 0.1 2.5 ± 0.5 2.0 ± 0.5 5.0 0.00
δ Vir 3602 ± 44 0.84 0.67 ± 0.09 −0.09 f 1.6 ± 0.1 2.5 ± 0.3 2.0 ± 0.5 3.0 0.03
δ Oph 3721 ± 47 1.02 0.89 ± 0.10 −0.03 g 1.6 ± 0.1 2.5 ± 0.5 2.0 ± 0.5 5.0 0.00
μ UMa 3793 ± 47 1.07 0.98 ± 0.08 0.00 h 1.5 ± 0.1 2.0 ± 0.5 6.0 0.00
α Lyn 3836 ± 47 0.98 1.02 ± 0.06 −0.26 i 1.8 ± 0.1 2.0 ± 0.5 5.0 0.08
α Tau 3871 ± 48 1.27 1.19 ± 0.10 0.00 f 1.5 ± 0.1 3.0 ± 1.0 2.0 ± 0.5 5.0 0.00
α Hya 4060 ± 50 1.35 1.20 ± 0.08 −0.12 i 1.5 ± 0.1 2.0 ± 0.5 5.0 0.00
α Boo 4226 ± 53 1.67 1.61 ± 0.05 −0.60 j 1.4 ± 0.1 2.2 ± 0.2 2.0 ± 0.5 6.0 0.18
α Ser 4558 ± 56 2.50 2.40 ± 0.10 0.03 i 1.2 ± 0.1 2.0 ± 0.5 5.0 0.00
β Gem 4858 ± 60 2.88 2.79 ± 0.10 −0.07 i 1.0 ± 0.1 2.0 ± 0.5 5.0 0.00

Reference.

(b)

typical uncertainty of ± 0.15;

(c)

Maria Bergemann, priv. comm.;

(d)

based on Tsuji (1985, 2008);

(e)

see text;

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