Table 6
Main results for the 42 OCs analysed, indicating, for each cluster, the number of stars from the sample detected in UVES and GIRAFFE; the number of stars with EW(Li) values; the number of stars selected as candidate members (including RV, astrometric and Li members, as well as the final members); and the number of Li-rich giant contaminants.
Clustera | UVES | GIRAFFE | Membership | Li-rich G | |||||
---|---|---|---|---|---|---|---|---|---|
All stars | With Li | All stars | With Li | RV | Gaia | Li | Final | outliers | |
NGC 6530 | 52 | 5 | 1931 | 1325 | 470 | 200 | 359 | 343 | 11 |
ρ Oph | 23 | 20 | 288 | 277 | 48 | 29 | 37 | 44 | 2 |
Trumpler 14 | 43 | 11 | 1859 | 1045 | 228 | 55 | 165 | 159 | 11 |
Cha I | 47 | 36 | 660 | 623 | 102 | 54 | 88 | 87 | 6 |
NGC 2244 | 8 | 6 | 444 | 385 | 143 | 79 | 123 | 116 | 1 |
NGC 2264 | 113 | 70 | 1740 | 1539 | 621 | 423 | 507 | 503 | 10 |
λ Ori | 116 | 103 | 720 | 675 | 207 | 142 | 163 | 161 | 3 |
Col 197 | 8 | 3 | 401 | 363 | 123 | 86 | 104 | 92 | 7 |
γ Vel | 79 | 50 | 1183 | 1140 | … | … | … | 234 | 1 |
NGC 2232 | 47 | 28 | 1822 | 1722 | 750 | 56 | 84 | 68 | 9 |
NGC 2547 | 54 | 33 | 423 | 372 | … | … | … | 151 | 0 |
IC 2391 | 48 | 26 | 386 | 374 | 56 | 27 | 37 | 35 | 6 |
IC 2602 | 131 | 89 | 1721 | 1651 | 309 | 43 | 59 | 55 | 24 |
IC 4665 | 34 | 30 | 533 | 514 | 233 | 29 | 51 | 33 | 0 |
NGC 2451 A/B | 90 | 70 | 1566 | 1537 | … | … | … | 106 | 10 |
NGC 6405 | 21 | 12 | 680 | 486 | 251 | 80 | 53 | 51 | 1 |
Blanco 1 | 37 | 31 | 426 | 373 | 142 | 119 | 101 | 98 | 0 |
NGC 6067 | 27 | 16 | 753 | 327 | 209 | 126 | 60 | 56 | 0 |
NGC 6649 | 6 | 0 | 277 | 62 | 42 | 21 | 4 | 2 | 0 |
NGC 2516 | 51 | 32 | 708 | 645 | 460 | 378 | 379 | 376 | 0 |
NGC 6709 | 10 | 10 | 720 | 590 | 322 | 71 | 53 | 49 | 10 |
NGC 6259 | 16 | 14 | 478 | 264 | 125 | 71 | 39 | 35 | 0 |
NGC 6705 | 49 | 31 | 1017 | 579 | 391 | 313 | 142 | 139 | 0 |
Berkeley 30 | 14 | 13 | 318 | 144 | 78 | 44 | 24 | 24 | 0 |
NGC 6281 | 16 | 7 | 304 | 214 | 82 | 38 | 23 | 23 | 1 |
NGC 3532 | 67 | 51 | 1094 | 809 | 518 | 411 | 323 | 384 | 11 |
NGC 4815 | 14 | 12 | 204 | 92 | 68 | 50 | 30 | 29 | 0 |
NGC 6633 | 57 | 38 | 1605 | 1463 | 617 | 35 | 62 | 67 | 9 |
NGC 2477 | 11 | 10 | 114 | 0 | 86 | 71 | 9 | 9 | 0 |
Trumpler 23 | 16 | 15 | 165 | 70 | 51 | 41 | 25 | 23 | 0 |
Berkeley 81 | 14 | 14 | 265 | 159 | 69 | 42 | 25 | 24 | 0 |
NGC 2355 | 11 | 11 | 197 | 149 | 119 | 129 | 87 | 86 | 0 |
NGC 6802 | 13 | 13 | 184 | 69 | 77 | 51 | 36 | 32 | 2 |
NGC 6005 | 19 | 19 | 541 | 298 | 174 | 112 | 55 | 49 | 3 |
Pismis 18 | 10 | 10 | 134 | 72 | 41 | 24 | 12 | 10 | 0 |
Melotte 71 | 9 | 9 | 111 | 0 | 71 | 64 | 4 | 4 | 0 |
Pismis 15 | 11 | 11 | 322 | 201 | 91 | 66 | 33 | 31 | 1 |
Trumpler 20 | 29 | 26 | 1184 | 404 | 451 | 367 | 116 | 104 | 0 |
Berkeley 44 | 7 | 7 | 86 | 73 | 39 | 33 | 31 | 30 | 0 |
NGC 2243 | 27 | 27 | 634 | 576 | 469 | 446 | 289 | 289 | 8 |
M67 | 42 | 36 | 95 | 85 | 109 | 89 | 96 | 96 | 0 |
Notes. (a)Regarding the clusters γ Vel, NGC 2547 and NGC 2451 A and B, we directly used the selections obtained by several studies listed in Table 1.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.