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Table 2.
Abundances obtained for each element analysed in each GCs.
| Cluster | Star | Flag Cu | [Cu/Fe] | [Y/Fe] | [Ba/Fe] | Flag La | [La/Fe] | Flag Eu | [Eu/Fe] |
|---|---|---|---|---|---|---|---|---|---|
| NGC 7099 | 954 | 0 | −0.65 | −0.20 | −0.32 | 1 | 0.19 | 0 | 0.79 |
| NGC 7099 | 3399 | 1 | −0.67 | −0.04 | −0.13 | 1 | 1.20 | 0 | 0.98 |
| NGC 7099 | 7414 | 0 | −0.56 | −0.13 | −0.17 | 1 | 0.28 | 1 | 0.66 |
| NGC 7099 | 9817 | 0 | −0.78 | −0.21 | 0.17 | 1 | 0.51 | 0 | 0.55 |
| NGC 7099 | 9956 | 0 | −0.57 | −0.25 | −0.20 | 1 | 0.46 | 1 | 0.72 |
| NGC 7099 | 10200 | 0 | −0.78 | −0.26 | −0.32 | 1 | 0.29 | 1 | 0.67 |
| ... | ... | ... | ... | ... | ... | ... | ... | ... | ... |
Notes. Stars for which we reported actual measurement and upper limits were flagged with 0 and 1, respectively. The star IDs were taken from Carretta et al. (2009, 2017). The full table is available at the CDS.
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