Table 5
Ages and metallicities of LMC star clusters derived from Washington photometry.
| Cluster name | Deprojected | Age (Gyr) | [Fe/H] | Reference |
| distance (°) | ||||
|
|
||||
| SL 8 | 4.2 | 1.6/1.8 | –0.5 | 1, 2 |
| NGC 1697 | 3.5 | 0.7 ± 0.1 | 0.0 | 3 |
| HS 38 | 4.0 | 0.4 ± 0.1 | –0.4 | 4 |
| KMHK 229 | 2.6 | 1.0 ± 0.2 | –0.4 | 4 |
| H88-26 | 3.3 | 0.8 ± 0.2 | –0.4 | 4 |
| H88-40 | 3.5 | 0.7 ± 0.2 | –0.4 | 4 |
| SL 126 | 8.9 | 1.9/2.2 | –0.45 | 1, 2 |
| SL 133 | 5.9 | 2.2 ± 0.3 | –0.7 | 3 |
| H88-55 | 3.3 | 0.5 ± 0.1 | –0.4 | 4 |
| SL 154 | 3.0 | 0.5 ± 0.1 | –0.4 | 4 |
| KMHK 506 | 2.2 | 0.6 ± 0.1 | –0.4 | 4 |
| SL 218 | 2.0 | 0.05 ± 0.01 | –0.4 | 5 |
| NGC 1836 | 1.9 | 0.4 ± 0.1 | 0.0 | 6 |
| BRHT 4b | 1.9 | 0.10 ± 0.02 | –0.4 | 5 |
| NGC 1839 | 1.9 | 0.12 ± 0.02 | –0.4 | 5 |
| NGC 1838 | 2.0 | 0.10 ± 0.02 | –0.4 | 5 |
| SL 229 | 2.1 | 0.3 ± 0.1 | –0.4 | 4 |
| SL 244 | 1.8 | 1.6/1.4 ± 0.3 | –0.7 | 1, 8 |
| BSDL 716 | 2.2 | 0.4 ± 0.1 | –0.4 | 4 |
| SL 262 | 8.6 | 2.1 | –0.55 | 1, 2 |
| HS 151 | 1.8 | 0.8 ± 0.2 | –0.4 | 4 |
| NGC 1860 | 1.4 | 0.25 ± 0.5 | 0.0 | 6 |
| H88-188 | 2.7 | 0.5 ± 0.1 | –0.4 | 4 |
| HS 154 | 2.5 | 0.5 ± 0.1 | –0.4 | 4 |
| SL 293 | 2.5 | 0.4 ± 0.1 | –0.4 | 4 |
| NGC 1863 | 1.4 | 0.04 ± 0.01 | –0.4 | 5 |
| SL 300 | 2.6 | 0.4 ± 0.1 | –0.4 | 4 |
| NGC 1865 | 1.3 | 0.9/0.5 ± 0.1 | –0.2 | 1, 6 |
| BSDL 1024 | 1.0 | 0.16 ± 0.03 | –0.4 | 4 |
| BSDL 1035 | 1.2 | 0.5 ± 0.1 | –0.4 | 4 |
| H88-245 | 0.7 | 0.16 ± 0.04 | –0.4 | 4 |
| SL 351 | 1.1 | 0.5 ± 0.1 | –0.4 | 4 |
| SL 359 | 1.3 | 1.8 ± 0.3 | –0.4 | 1, 8 |
| SL 388 | 7.0 | 2.6/2.2 | –0.65 | 1, 2 |
| IC 2134 | 6.9 | 1.0 | – | 2 |
| SL 451 | 7.0 | 2.2 | –0.7 | 1, 2 |
| SL 446A | 2.0 | 2.3 ± 0.3 | –0.8 | 1, 8 |
| SL 444 | 2.0 | 0.5 ± 0.1 | –0.4 | 6 |
| SL 490 | 4.8 | 1.3 ± 0.3 | –0.4 | 7 |
| SL 505 | 2.5 | 1.6/1.2 ± 0.3 | –0.6 | 1, 8 |
| SL 510 | 1.4 | 0.13 ± 0.03 | –0.4 | 4 |
| SL 509 | 6.6 | 1.4/1.2 | –0.85 | 1, 2 |
| LW 224 | 3.0 | 0.7 ± 0.1 | 0.0 | 6 |
| LW 231 | 6.7 | 0.8 ± 0.3 | –0.4 | 7 |
| NGC 1997 | 7.1 | 2.6 ± 0.5 | –0.7 | 3 |
| SL 548 | 3.0 | 0.4 ± 0.1 | 0.0 | 6 |
| SL 555 | 3.1 | 1.6/1.7 ± 0.3 | –0.7 | 1, 8 |
| SL 549 | 5.9 | 1.3/2.0 ± 0.3 | –0.9 | 1, 8 |
| KMHK 1045 | 1.9 | 0.6 ± 0.1 | –0.4 | 4 |
| KMHK 1055 | 2.0 | 1.0 ± 0.2 | –0.4 | 4 |
| SL 588 | 1.7 | 0.4 ± 0.1 | –0.4 | 4 |
| NGC 2093 | 2.0 | 0.25 ± 0.05 | –0.4 | 4 |
| SL 663 | 4.8 | 3.0 ± 0.8 | –0.7 | 3 |
| SL 674 | 3.9 | 2.1/2.2 ± 0.3 | –0.9 | 1, 8 |
| SL 678 | 4.0 | 1.8 ± 0.3 | –0.8 | 8 |
| H88-333 | 2.3 | 0.4 ± 0.1 | –0.4 | 4 |
| BSDL 2995 | 2.4 | 1.0 ± 0.2 | –0.4 | 4 |
| H7 | 3.2 | 1.4 | – | 1 |
| SL 769 | 2.9 | 1.8 | –0.5 | 2 |
| KMHK 1507 | 3.5 | 0.8 ± 0.3 | –0.4 | 7 |
| SL 775 | 3.5 | 0.6 ± 0.3 | –0.4 | 7 |
| OHSC 28 | 8.3 | 2.4 ± 0.5 | –0.7 | 3 |
| NGC 2161 | 5.9 | 1.1 ± 0.3 | –0.7 | 9 |
| NGC 2153 | 4.6 | 1.3 | – | 1 |
| NGC 2155 | 5.4 | 3.2 ± 0.6 | –0.9 | 10 |
| SL 817 | 3.6 | 2.5/1.5 | –0.5 | 1, 2 |
| ESO 121-03 | 10.4 | 8.5 | –1.05 | 1, 2 |
| SL 842 | 8.1 | 1.9/2.2 | –0.6 | 1, 2 |
| NGC 2213 | 4.6 | 1.5 | –0.4 | 11 |
| SL 862 | 4.7 | 1.8 | –0.85 | 1, 2 |
| OHSC 33 | 6.2 | 1.2/1.4 | –1.0 | 1, 2 |
| SL 874 | 4.9 | 1.5 ± 0.3 | –0.7 | 9 |
| KMHK 1719 | 5.1 | 1.4 ± 0.3 | –0.6 | 9 |
| LW 469 | 5.9 | 0.6 ± 0.1 | –0.4 | 4 |
| SL 896 | 6.4 | 2.3 ± 0.3 | –0.6 | 10 |
| OHSC 37 | 9.4 | 2.1 | –0.65 | 1, 2 |
References. (1) Geisler et al. (1997); (2) Bica et al. (1998); (3) Piatti et al. (2009); (4) Piatti (2012); (5) Piatti et al. (2003b); (6) Piatti et al. (2003a); (7) Palma et al. (2011); (8) Geisler et al. (2003); (9) Piatti et al. (2011); (10) Piatti et al. (2002); (11) Geisler (1987).
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.