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Table 2.
Stellar parameters adopted with Turbospectrum and with SYNTHE.
| Turbospectrum |
SYNTHE |
|||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| Star | Teff | log g | [Fe/H] | vt | Ref. | Teff | log g | [Fe/H] | vt | Ref. |
| HD 19445 | 6070 | 4.4 | −2.15 | 1.3 | 1 | 6050 | 4.5 | −2.00 | 1.0 | 6 |
| HD 84937 | 6300 | 4.0 | −2.25 | 1.3 | 2 | 6300 | 4.0 | −2.25 | 1.3 | 3 |
| HD 94028 | 6050 | 4.3 | −1.40 | 1.2 | 3 | 6050 | 4.3 | −1.40 | 1.2 | 3 |
| HD 140283 | 5750 | 3.7 | −2.57 | 1.4 | 4 | 5700 | 3.6 | −2.60 | 1.3 | 3 |
| HD 160617 | 5950 | 3.9 | −1.80 | 1.3 | 5 | 6000 | 3.8 | −1.80 | 1.2 | 6 |
Notes. [Fe/H] = log(NFe/NH)star − log(NFe/NH)Sun.
References. (1) Roederer et al. (2018a); (2) Spite et al. (2017); (3) Peterson et al. (2017); (4) Siqueira Mello et al. (2015); (5) Roederer & Lawler (2012); (6) Peterson & Kurucz (2015).
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