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Table 9.

Abundance ratios of open clusters in the GES sample.

Cluster # stars [Y/Mg] [Y/Al] [Y/TiI] [Y/TiII] [Y/Ca] [Y/Si]
(dex) (dex) (dex) (dex) (dex) (dex)
Berkeley 31 5 (G) −0.01 ± 0.03 0.02 ± 0.03 0.01 ± 0.04 −0.07 ± 0.04 0.06 ± 0.04 0.03 ± 0.04
Berkeley 36 5 (G) −0.05 ± 0.06 −0.07 ± 0.06 0.00 ± 0.07 −0.04 ± 0.07 0.13 ± 0.06 −0.02 ± 0.06
Berkeley 44 7 (G) 0.14 ± 0.07 0.19 ± 0.07 0.13 ± 0.08 −0.04 ± 0.14 0.26 ± 0.07 0.18 ± 0.07
Berkeley 81 13 (G) 0.09 ± 0.03 0.07 ± 0.03 0.13 ± 0.05 0.17 ± 0.05 0.19 ± 0.04 0.08 ± 0.04
M 67 3 (G) 0.00 ± 0.01 0.00 ± 0.01 0.00 ± 0.01 0.00 ± 0.01 0.00 ± 0.01 0.00 ± 0.01
Melotte 71 4 (G) 0.07 ± 0.01 0.15 ± 0.01 0.13 ± 0.02 0.09 ± 0.01 0.03 ± 0.01 0.09 ± 0.03
NGC 2243 17 (16 G, 1 SG) −0.04 ± 0.03 0.00 ± 0.03 0.00 ± 0.05 −0.04 ± 0.04 −0.02 ± 0.09 −0.01 ± 0.03
NGC 2420 28 (24 G, 4 SG) 0.07 ± 0.03 0.13 ± 0.03 0.08 ± 0.03 0.04 ± 0.03 0.07 ± 0.03 0.08 ± 0.03
NGC 4815 6 (G) 0.11 ± 0.09 0.16 ± 0.08 0.19 ± 0.10 0.10 ± 0.08 0.12 ± 0.09 0.08 ± 0.07
NGC 6005 9 (G) −0.01 ± 0.02 0.02 ± 0.02 0.03 ± 0.03 0.02 ± 0.02 0.05 ± 0.02 −0.05 ± 0.02
NGC 6067 12 (G) 0.08 ± 0.04 0.03 ± 0.05 0.06 ± 0.05 0.13 ± 0.04 0.05 ± 0.07 0.02 ± 0.04
NGC 6259 12 (G) −0.05 ± 0.02 −0.05 ± 0.02 0.00 ± 0.04 0.07 ± 0.03 0.04 ± 0.02 −0.08 ± 0.02
NGC 6633 3 (G) 0.08 ± 0.02 0.18 ± 0.02 0.19 ± 0.02 0.11 ± 0.01 0.09 ± 0.01 0.07 ± 0.01
NGC 6705 28 (G) −0.03 ± 0.03 −0.10 ± 0.03 0.05 ± 0.04 0.08 ± 0.04 0.02 ± 0.04 −0.09 ± 0.03
NGC 6802 10 (G) 0.17 ± 0.02 0.14 ± 0.02 0.23 ± 0.03 0.10 ± 0.02 0.24 ± 0.02 0.13 ± 0.02
Rup 134 16 (G) −0.08 ± 0.02 −0.08 ± 0.02 −0.03 ± 0.02 −0.04 ± 0.02 0.04 ± 0.02 −0.14 ± 0.02
Pismis 18 6 (G) 0.05 ± 0.04 0.10 ± 0.04 0.13 ± 0.04 0.06 ± 0.04 0.12 ± 0.04 0.00 ± 0.04
Trumpler 20 34 (G) 0.12 ± 0.02 0.16 ± 0.02 0.17 ± 0.02 0.08 ± 0.02 0.15 ± 0.02 0.04 ± 0.02
Trumpler 23 10 (G) −0.05 ± 0.04 −0.02 ± 0.04 0.05 ± 0.06 0.01 ± 0.04 0.11 ± 0.05 −0.10 ± 0.04

Notes. G: giants, SG: sub-giants.

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