Table 3
LTE and NLTE abundances from individual lines in the sample stars.
| Atom | λ | E exc | log gf | log Γ6/NH | EW |
|
|
|
|
|||||||
| (Å) | (eV) | (rad/s cm3) | (mÅ) | LTE | NLTE | ||
|
|
|||||||
| ET0381 | |||||||
| Na I | 5889.95 | 0.00 | 0.12 | −7.670 | 173.0 | 3.51 | 3.19 |
| Na I | 5895.92 | 0.00 | −0.19 | −7.670 | 143.0 | 3.35 | 3.07 |
| Mg I | 5172.68 | 2.71 | −0.45 | −7.267 | 197.2 | 5.04 | 5.06 |
| Mg I | 5183.60 | 2.72 | −0.24 | −7.267 | 204.8 | 4.90 | 4.93 |
| Mg I | 5528.41 | 4.35 | −0.50 | −7.180 | 59.5 | 4.99 | 5.00 |
| Al I | 3961.52 | 0.01 | −0.34 | −7.315 | −1 | 2.72 | 2.82 |
Notes. This table is available in its entirety in a machine-readable form at the CDS. A portion is shown here for guidance regarding its form and content. Γ6 corresponds to 10 000 K. The sources of the observed equivalent widths, EWs, are indicated in Table 4. EW = −1 means using spectral synthesis.
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