Table 8
Atmospheric parameters and abundances of Fe and Ti of stars in IC 2391.
| ID | Teff | log g | ξ | [Fe/H]I | [Fe/H]II | [Ti/H]I | [Ti/H]II |
|---|---|---|---|---|---|---|---|
| PMM 1142 | 5400 ± 100 | 4.28 ± 0.07 | 0.95 ± 0.10 | 0.00 ± 0.02 ± 0.07 | +0.11 ± 0.03 ± 0.06 | +0.04 ± 0.02 ± 0.10 | +0.06 ± 0.03 ± 0.05 |
| PMM 665 | 5425 ± 100 | 4.47 ± 0.05 | 1.01 ± 0.15 | +0.08 ± 0.02 ± 0.07 | +0.14 ± 0.05 ± 0.06 | +0.10 ± 0.02 ± 0.11 | +0.11 ± 0.05 ± 0.05 |
| PMM 4362 | 5550 ± 100 | 4.35 ± 0.05 | 0.97 ± 0.15 | +0.13 ± 0.02 ± 0.08 | +0.14 ± 0.04 ± 0.06 | +0.09 ± 0.03 ± 0.11 | +0.12 ± 0.02 ± 0.05 |
Notes. Atmospheric parameters and abundances of Fe and Ti derived with the same methodology as in Paper I of the stars from D’Orazi et al. (2017). The uncertainties are due to the dispersion among different atomic lines (first value) and to uncertainties on the stellar parameters (second value).
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