Table 6
Derived elemental abundances for the individual stars in NGC 6752.
Group | Star ID | log ε(Mg) | log ε(Al) | log ε(Na) | log ε(Li) | Pop | ||
NLTE | LTE | NLTE | NLTE | |||||
|
||||||||
RGB | 540 | 6.11 ± 0.07 | 5.27 ± 0.05 | 4.74 ± 0.10 | 1.22 ± 0.05 | I | ||
548 | 5.92 ± 0.09 | 5.83 ± 0.07 | 4.98 ± 0.10 | <0.60a | E | |||
566 | 6.12 ± 0.07 | 5.00 ± 0.05 | 4.34 ± 0.10 | 0.95 ± 0.08 | P | |||
574 | 6.15 ± 0.07 | 4.83 ± 0.10a | 4.25 ± 0.10 | 0.99 ± 0.07 | P | |||
581 | 6.14 ± 0.07 | 5.35 ± 0.05 | 4.79 ± 0.10 | 0.99 ± 0.07 | I | |||
588 | 6.06 ± 0.07 | 5.38 ± 0.05 | 4.74 ± 0.10 | 0.99 ± 0.07 | I | |||
|
||||||||
bRGB | 1406 | 6.17 ± 0.07 | 4.50 ± 0.07 | 1.01 ± 0.13 | P | |||
1483 | 6.11 ± 0.07 | 4.88 ± 0.05 | 4.63 ± 0.07 | 1.13 ± 0.10 | ||||
1522 | 6.23 ± 0.07 | 4.44 ± 0.07 | 1.11 ± 0.11 | P | ||||
1665 | 6.21 ± 0.07 | 5.08 ± 0.05 | 4.71 ± 0.07 | 1.16 ± 0.09 | ||||
|
||||||||
SGB | 3081 | 6.05 ± 0.07 | 4.58 ± 0.07 | 2.11 ± 0.05 | ||||
|
||||||||
TOP | 3988 | 6.05 ± 0.11 | 4.58 ± 0.07 | 2.30 ± 0.06 | ||||
4096 | 6.02 ± 0.11 | no reliable | 4.71 ± 0.07 | 2.34 ± 0.07 | ||||
4138 | 6.05 ± 0.11 | abundance | 4.95 ± 0.07 | 2.03 ± 0.10 | ||||
4383 | 6.12 ± 0.11 | 4.31 ± 0.07 | 2.21 ± 0.07 | |||||
4428 | 6.09 ± 0.11 | 4.30 ± 0.07 | 2.13 ± 0.10 |
Notes.For magnesium two Mg I lines: 5528 and 5711 Å, for aluminium we used the Al I doublet at 6696–6698 Å, and for sodium we used the Na I doublet at 5682–5688 Å, for the RGB we also included the Na I doublet at 6154.2–6160.7 Å. Lithium abundances were derived using the Li I line at 6707 Å. The last column gives the population: P for primordial, I for intermediate and E for extreme following Carretta et al. (2009).
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