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Table 1.

Sample of stars with their physical parameters, including LTE and NLTE abundances of Mn.

Star Teff log g [Fe/H] Vmic [Mn/Fe]
K dex km s−1 LTE NLTE Source
Dwarfs
HD 3567 6035 4.08 −1.29 1.5 −0.43 −0.29 c
HD 6582 5387 4.45 −0.83 0.9 −0.21 −0.13 a
HD 19445 5982 4.38 −2.10 1.4 −0.40 −0.21 c
HD 22879 5792 4.30 −0.95 1.2 −0.24 −0.15 c
HD 84937 6350 4.10 −2.15 1.4 −0.34 −0.16 b
HD 106038 5950 4.33 −1.45 1.1 −0.22*/−0.4 −0.15 c
HD 121004 5711 4.46 −0.71 0.7 0.28* 0.23 c
HD 122196 6048 3.89 −1.75 1.2 −0.45 −0.28 c
BD 133442 6450 4.42 −2.47 1.5 −0.38* −0.32 c
HD 134169 5930 3.98 −0.86 1.8 −0.21 −0.10 a
HD 140283 5777 3.70 −2.38 1.3 −0.51 −0.21 b,c
HD 142267 5807 4.42 −0.46 1.0 −0.17 −0.10 a
HD 144061 5815 4.44 −0.31 1.2 −0.01 0.04 a
HD 148816 5880 4.07 −0.78 1.2 −0.32 −0.22 a
HD 157466 5990 4.38 −0.44 1.1 −0.23 −0.15 a
HD 158226 5805 4.12 −0.56 1.1 −0.18 −0.09 a
HD 160693 5850 4.31 −0.60 1.2 −0.18 −0.09 a
HD 160933 5765 3.85 −0.27 1.2 −0.24 −0.15 a
HD 170357 5665 4.07 −0.50 1.2 −0.24 −0.14 a
HD 171620 6115 4.20 −0.50 1.4 −0.17 −0.08 a
HD 182807 6100 4.21 −0.33 1.4 −0.13 −0.05 a
HD 184448 5765 4.16 −0.43 1.2 0.01 0.07 a,c
HD 186379 5865 3.93 −0.41 1.2 −0.20 −0.10 a
HD 198300 5890 4.31 −0.60 1.2 −0.04 0.04 a
HD 200580 5940 3.96 −0.82 1.4 0.09 0.19 a
HD 204155 5815 4.09 −0.66 1.2 −0.34 −0.21 a
HD 208906 6025 4.37 −0.76 1.4 −0.22 −0.11 a
HD 215257 6030 4.28 −0.58 1.4 −0.26 −0.15 a
HD 218209 5665 4.40 −0.60 1.1 −0.05 0.04 a
HD 221876 5865 4.29 −0.60 1.2 −0.32 −0.22 a
HD 224930 5480 4.45 −0.66 0.9 −0.33 −0.24 a
G 64−12 6464 4.30 −3.12 1.5 −0.40* −0.32 b,c
Giants
HD 74462 4590 1.98 −1.43 1.1 −0.36 −0.07 c
HD 115444 4785 1.71 −2.87 2.1 −0.75 −0.36 d
HD 122563 4665 1.65 −2.50 1.8 −0.71 −0.22 b,c
HD 126238 4900 2.02 −1.85 1.5 −0.45 −0.14 c
HD 126587 4950 2.36 −2.86 1.7 −0.70 −0.27 c
HD 128279 5200 1.73 −2.13 1.3 −0.55* −0.52 d
HD 175305 5100 2.70 −1.34 1.2 −0.23 0.02 c
HD 186478 4730 1.56 −2.33 1.8 −0.53 −0.21 d
BD +541323 5213 2.20 −1.55 1.5 −0.55 −0.25 d
HE 0315+0000 5050 2.47 −2.67 1.6 −0.55 −0.11 c

Notes. The NLTE abundances are averaged over Mn I and Mn II lines, because of the weak ionisation imbalance. LTE abundances are given either for Mn I or Mn II lines (marked with an asterisk), depending on the available data. The lines of the 4030 Å triplet are excluded for giants, since they are sensitive to convection effects (see Paper I).

References. a: Gehren et al. (2004), b: Bergemann et al. (2012), c: Hansen et al. (2013), d: Hansen et al. (2012), Hansen & Primas (2011).

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