Table 8
Abundances of light elements for the four clusters in common between our study and those of Sakari et al. (2013) and Colucci et al. (2017).
| NGC 104 | NGC 362 | NGC 6388 | NGC 6752 | NGC 7078 | ||
|
|
||||||
| [Na/Fe] | C2009 (rms) | 0.53 (0.15) | 0.19 (0.19) | 0.59 (0.16) | 0.33 (0.27) | 0.20 (0.25) |
| Colucci et al. (2017) | 0.24 ± 0.08 | −0.02 ± 0.10 | −0.17 ± 0.36 | 0.04 ± 0.07 | ... | |
| Sakari et al. (2013) | 0.38 ± 0.12 | ... | ... | ... | 0.90 ± 0.40 | |
| Std analysis | 0.42 | −0.05 | 0.36 | 0.30 | 0.15 | |
| [Mg/Fe] | C2009 (rms) | 0.52 (0.03) | 0.33 (0.04) | 0.21 (0.07) | 0.50 (0.05) | 0.45 (0.19) |
| Colucci et al. (2017) | 0.29 ± 0.08 | 0.07 ± 0.05 | −0.02 ± 0.10 | 0.06 ± 0.07 | ... | |
| Sakari et al. (2013) | 0.42 ± 0.14 | ... | ... | ... | −0.15 ± 0.21 | |
| Std analysis | 0.44 | 0.15 | 0.11 | 0.39 | 0.18 | |
| Kurucz line list | 0.54 | 0.25 | 0.19 | 0.44 | 0.24 | |
Notes. For convenience we repeat our abundance measurements from Tables 3 (standard analysis) and B.2 (Kurucz line list). For Carretta et al. (2009b) we include the rms dispersions as given in their Table 10. (Note that the data for NGC 362 are from Carretta et al. 2013.)
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