Table 1
West halo clusters with known parameters, selected as a subsample of Bica et al. (2008) using our definition.
| Cluster | Other names | RA | Dec | a | [Fe/H] | Age | Dist. | Ref. | ||
| h m s | ° ′ ″ | (deg) | (Gyr) | (kpc) | ||||||
|
|
||||||||||
| Paper I results (homogeneous scale with this work) | ||||||||||
|
|
||||||||||
| L 3 | ESO28SC13 | 00:18:25 | −74:19:07 | 2.9 | −0.65 |
1.01 |
54.2 ± 1.5 | 1, 1, 1 | ||
| HW 1 | – | 00:18:27 | −73:23:42 | 3.4 | −1.43 |
3.90 |
58.4 ± 1.6 | 1, 1, 1 | ||
| L 2 | – | 00:12:55 | −73:29:15 | 3.9 | −1.58 |
3.54 |
56.9 ± 1.6 | 1, 1, 1 | ||
| AM-3 | ESO28SC4 | 23:48:59 | −72:56:43 | 7.3 | −0.98 |
4.88 |
63.2 |
1, 1, 1 | ||
|
|
||||||||||
| Other references | ||||||||||
|
|
||||||||||
| NGC 152 | K10, L15, ESO28SC24 | 00:32:56 | −73:06:58 | 2.0 | −1.13 ± 0.15 | 9.3 ± 1.7 | 62.7 ± 5.7 | 2, 2, 3 | ||
| K 9 | L13 | 00:30:00 | −73:22:45 | 2.2 | −1.24 | 4.7 | − | 4, 4, − | ||
| K 6 | L9, ESO28SC20 | 00:25:26 | −74:04:33 | 2.4 | −0.7 | 1.6 ± 0.4 | − | 5, 5, − | ||
| K 5 | L7, ESO28SC18 | 00:24:43 | −73:45:18 | 2.5 | −0.6 | 2.0 | − | 6, 7, − | ||
| K 4 | L6, ESO28SC17 | 00:24:43 | −73:45:18 | 2.7 | −0.9 | 3.3 | − | 6,7,− | ||
| K 1 | L4, ESO28SC15 | 00:21:27 | −73:44:55 | 2.8 | −0.9 | 3.3 | − | 6, 7, − | ||
| L 5 | ESO28SC16 | 00:21:27 | −73:44:55 | 3.0 | −1.2 | 4.1 | − | 6, 7, − | ||
| K 7 | L11, ESO28SC22 | 00:27:46 | −72:46:55 | 3.0 | −0.8 | 3.5 | − | 8, 8, − | ||
| K 3 | L8, ESO28SC19 | 00:24:47 | −72:47:39 | 3.3 | −1.12 | 6.5 | 56.7 ± 1.9 | 9, 9, 3 | ||
| NGC 121 | K2, L10, ESO50SC12 | 00:26:47 | −71:32:12 | 4.8 | −1.2 ± 0.12 | 10.5 ± 0.5 | 59.6 ± 1.8 | 8, 10, 3 | ||
| L 1 | ESO28SC8 | 00:03:54 | −73:28:19 | 5.0 | −1.0 | 7.5 | 53.2 ± 0.9 | 11, 11, 3 | ||
Notes. The semi-major axis a is calculated as in Paper I, and the table is sorted by this parameter. References for metallicity, age, and distance are indicated in the last column and notes are at the bottom of the table.
Reference. (1) Paper I; (2) Dias et al. (2010); (3) Crowl et al. (2001); (4) Mighell et al. (1998); (5) Piatti et al. (2005a); (6) Piatti et al. (2005b); (7) Parisi et al. (2009); (8) Da Costa & Hatzidimitriou (1998); (9) Glatt et al. (2008b); (10) Glatt et al. (2008a); (11) Glatt et al. (2009).
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