Table 10.
Comparison of temperature, surface gravity, microturbulent velocity, and iron abundance with those of Holanda et al. (2019).
| Star | Holanda19 ( * ) |
This work |
||||||
|---|---|---|---|---|---|---|---|---|
| Teff (K) | log g | ξ (km s−1) | [Fe/H] ( * *) | Teff (K) | log g | ξ (km s−1) | [Fe/H] | |
| 14 | 4150 | 1.10 | 2.36 | −0.29 | 4024 ± 52 | 0.77 ± 0.14 | 1.71 | −0.31 ± 0.07 |
| 34 | 4850 | 1.10 | 3.00 | −0.20 | 4810 ± 45 | 1.08 ± 0.09 | 2.35 | −0.19 ± 0.05 |
| 43 | 4350 | 1.60 | 2.45 | −0.27 | 4251 ± 21 | 1.10 ± 0.06 | 1.69 | −0.31 ± 0.03 |
| 50 | 4000 | 0.70 | 2.31 | −0.32 | 3948 ± 34 | 0.70 ± 0.10 | 1.67 | −0.34 ± 0.05 |
| 60 | 4020 | 1.03 | 2.54 | −0.34 | 4200 ± 45 | 1.00 ± 0.13 | 1.72 | −0.27 ± 0.06 |
Notes. ( * )Typical uncertainties are Δ Teff = 70–100 K, Δ log g = 0.1–0.2 dex, Δ ξ = 0.20 km s−1, and Δ [Fe/H] = 0.1 dex.
( * *)The iron abundance, is rescaled to the solar reference used in this work (Grevesse et al. 2007).
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