Table B.1
Data for star clusters that have been searched for the Na-O anti-correlation or multiple populations in the colour-magnitude diagram.
Class | Object | Alt. name | M ∗ | r h a | C 5 b | Age | [Fe/H] | MPsc | Ref. |
(105 M⊙) | (pc) | (Gyr) | |||||||
|
|||||||||
GC | NGC 104 | 47 Tuc | 6.46 | 7.1 | 0.92 | 12.8 | –0.76 | Y | 1, 2, 3, 4 |
GC | NGC 288 | Melotte 3 | 0.46 | 9.8 | 0.05 | 12.2 | –1.32 | Y | 1, 2, 3, 4 |
GC | NGC 362 | Dunlop 62 | 2.5 | 3.5 | 0.72 | 10 | –1.26 | Y | 2, 3, 4, 5 |
GC | NGC 1261 | Caldwell 87 | 3.41 | 5.5 | 0.62 | 10.24 | –1.08 | Y | 2, 4, 6, 7 |
GC | NGC 1851 | Dunlop 508 | 5.51 | 3.05 | 1.81 | 7.64 | –1.13 | Y | 2, 4, 6, 8 |
GC | NGC 1904 | M79 | 1.45 | 4.1 | 0.50 | 12.0 | –1.58 | Y | 1, 2, 9 |
GC | NGC 2298 | Dunlop 578 | 0.85 | 3.1 | 0.16 | 12.4 | –1.98 | Y | 2, 4, 6, 8 |
GC | NGC 2808 | Dunlop 265 | 12.3 | 3.8 | 3.24 | 11.2 | –1.18 | Y | 1, 2, 3, 4 |
GC | NGC 3201 | Dunlop 445 | 1.1 | 7.5 | 0.15 | 11.1 | –1.51 | Y | 1, 2, 4, 10 |
GC | NGC 4590 | M68 | 1.07 | 7.7 | 0.14 | 12.7 | –2.27 | Y | 1, 2, 3, 4 |
GC | NGC 4833 | Dunlop 164 | 4.10 | 7.9 | 0.52 | 12.5 | –1.71 | Y | 2, 4, 6, 7 |
GC | NGC 5024 | M53 | 8.26 | 11.6 | 0.71 | 12.7 | –1.86 | Y | 2, 4, 6, 7 |
GC | NGC 5053 | 1.25 | 22.5 | 0.056 | 12.3 | –1.98 | Y | 2, 4, 6, 7 | |
GC | NGC 5272 | M3 | 4.68 | 11.7 | 0.40 | 11.4 | –1.34 | Y | 2, 3, 4, 7 |
GC | NGC 5286 | 7.13 | 4.2 | 1.69 | 12.5 | –1.41 | Y | 2, 3, 4, 7 | |
GC | NGC 5466 | 1.79 | 18.2 | 0.098 | 13.6 | –2.20 | Y | 2, 4, 6, 7 | |
GC | NGC 5897 | 2.11 | 12.7 | 0.17 | 12.3 | –1.73 | Y | 2, 4, 6, 7 | |
GC | NGC 5904 | M5 | 3.89 | 6.6 | 0.59 | 11.5 | –1.33 | Y | 1, 2, 3, 4 |
GC | NGC 5927 | 3.38 | 4.2 | 0.81 | 12.7 | –0.64 | Y | 2, 4, 6, 7 | |
GC | NGC 5986 | 5.99 | 5.04 | 1.19 | 12.2 | –1.35 | Y | 2, 4, 6, 7 | |
GC | NGC 6093 | M80 | 5.02 | 3.02 | 1.66 | 12.5 | –1.47 | Y | 2, 4, 6, 7 |
GC | NGC 6101 | Caldwell 107 | 1.0 | 8.00 | 0.13 | 12.5 | –1.76 | Y | 2, 4, 7, 11 |
GC | NGC 6121 | M4 | 1.17 | 4.7 | 0.25 | 13.1 | –1.98 | Y | 1, 2, 3, 4 |
GC | NGC 6139 | 3.80 | 4.2 | 0.90 | 11.6 | –1.58 | Y | 1, 2, 12 | |
GC | NGC 6144 | 1.69 | 7.17 | 0.24 | 13.8 | –1.56 | Y | 2, 4, 6, 7 | |
GC | NGC 6171 | M107 | 1.17 | 5.5 | 0.21 | 13.4 | –1.03 | Y | 1, 2, 4, 13, 14, |
GC | NGC 6205 | M13 | 7.75 | 5.93 | 1.31 | 11.7 | –1.33 | Y | 2, 4, 6, 7 |
GC | NGC 6218 | M12 | 0.74 | 4.2 | 0.18 | 13.4 | –1.43 | Y | 1, 2, 3, 4 |
GC | NGC 6254 | M10 | 1.53 | 4.2 | 0.36 | 12.4 | –1.57 | Y | 1, 2, 4, 15 |
GC | NGC 6304 | 2.17 | 4.14 | 0.52 | 13.6 | –0.66 | Y | 2, 4, 6, 7 | |
GC | NGC 6341 | M92 | 4.89 | 4.19 | 1.17 | 13.2 | –2.16 | Y | 2, 4, 6, 7 |
GC | NGC 6352 | 0.37 | 5.68 | 0.065 | 12.7 | –0.70 | Y | 2, 4, 7, 16 | |
GC | NGC 6362 | 0.81 | 7.70 | 0.11 | 13.6 | –0.99 | Y | 2, 4, 7, 16 | |
GC | NGC 6366 | 0.30 | 5.05 | 0.058 | 13.3 | –0.73 | Y | 2, 4, 7, 16 | |
GC | NGC 6388 | 12 | 2.5 | 4.8 | 11.7 | –0.45 | Y | 1, 2, 4, 17 | |
GC | NGC 6397 | 1.1 | 3.3 | 0.33 | 13.4 | –1.99 | Y | 1, 2, 4, 18 | |
GC | NGC 6441 | 9.55 | 3.3 | 2.92 | 11.2 | –0.44 | Y | 1, 2, 3, 4 | |
GC | NGC 6496 | 2.00 | 5.70 | 0.35 | 12.4 | –0.70 | Y | 2, 4, 6, 7 | |
GC | NGC 6535 | 0.20 | 2.86 | 0.070 | 10.5 | –1.51 | Y | 2, 4, 6, 7 | |
GC | NGC 6541 | 5.72 | 3.93 | 1.45 | 12.9 | –1.53 | Y | 2, 4, 6, 7 | |
GC | NGC 6584 | 3.03 | 4.87 | 0.62 | 11.3 | –1.30 | Y | 2, 4, 6, 7 | |
GC | NGC 6624 | 2.57 | 3.20 | 0.80 | 12.5 | –0.70 | Y | 2, 4, 6, 7 | |
GC | NGC 6637 | M69 | 2.00 | 3.66 | 0.55 | 13.1 | –0.78 | Y | 2, 4, 7, 19 |
GC | NGC 6652 | 1.09 | 2.37 | 0.46 | 12.0 | –0.97 | Y | 2, 4, 6, 7 | |
GC | NGC 6656 | M22 | 6.44 | 5.32 | 1.21 | 12.7 | –1.49 | Y | 2, 4, 6, 7 |
GC | NGC 6681 | M70 | 1.79 | 3.16 | 0.57 | 12.8 | –1.35 | Y | 2, 4, 6, 7 |
GC | NGC 6715 | M54 | 12.9 | 10.7 | 1.20 | 10.8 | –1.25 | Y | 2, 3, 4, 7 |
GC | NGC 6717 | 0.48 | 2.39 | 0.20 | 13.2 | –1.09 | Y | 2, 4, 6, 7 | |
GC | NGC 6723 | 3.57 | 6.58 | 0.54 | 13.1 | –0.96 | Y | 2, 4, 6, 7 | |
GC | NGC 6752 | 2.82 | 3.8 | 0.75 | 13.8 | –1.55 | Y | 1, 2, 3, 4 | |
GC | NGC 6779 | M56 | 2.30 | 5.11 | 0.45 | 13.7 | –2.00 | Y | 2, 4, 6, 7 |
GC | NGC 6809 | M55 | 0.55 | 7.6 | 0.07 | 13.8 | –1.93 | Y | 1, 2, 3, 4 |
GC | NGC 6838 | M71 | 0.20 | 3.3 | 0.06 | 12.7 | –0.82 | Y | 1, 2, 3, 4 |
GC | NGC 6934 | 2.95 | 5.32 | 0.55 | 11.1 | –1.32 | Y | 2, 4, 6, 7 | |
GC | NGC 6981 | M72 | 1.68 | 7.82 | 0.21 | 10.9 | –1.21 | Y | 2, 4, 6, 7 |
GC | NGC 7078 | M15 | 5.13 | 5.1 | 1.00 | 13.6 | –2.33 | Y | 1, 2, 3, 4 |
GC | NGC 7089 | M2 | 5.75 | 6.03 | 0.95 | 11.8 | –1.31 | Y | 2, 3, 4, 7 |
GC | NGC 7099 | M30 | 1.45 | 4.1 | 0.35 | 14.6 | –2.33 | Y | 1, 2, 3, 4 |
GC | Ruprecht 106 | 0.68 | 11 | 0.06 | 12 | –1.5 | N | 2, 20 | |
GC | Terzan 7 | 0.39 | 8.7 | 0.04 | 7.4 | –0.12 | N | 1, 2, 21, 22 | |
GC | Palomar 12 | 0.28 | 16 | 0.024 | 8.6 | –0.81 | N | 1, 2, 21 | |
OC | Berkley 39 | 0.2 | 11 | 0.018 | 6 | –0.21 | N | 23, 24 | |
OC | Collinder 261 | 0.01 | 2d | 0.005 | 6 | –0.03 | N | 24, 25, 26 | |
OC | Melotte 25 | Hyades | 0.004 | 3.7 | 0.001 | 0.6 | +0.13 | N | 27, 28, 29, 30 |
OC | Melotte 111 | Coma Berenices | 0.001 | 3.5 | 0.0003 | 0.5 | +0.07 | N | 27, 29, 31, 32 |
OC | NGC 752 | 0.001 | 1.4 | 0.0009 | 1.12 | –0.02 | N | 29, 33, 34 | |
OC | NGC 1817 | Collinder 4a | 0.02 | 7 | 0.002 | 1 | –0.11 | N | 27, 32, 34, 35, 36 |
OC | NGC 2360 | Melotte 64 | 0.018 | 2 | 0.009 | 0.56 | –0.07 | N | 29, 34, 37 |
OC | NGC 2506 | Collinder 170 | 0.03 | 15 | 0.002 | 1.11 | –0.19 | N | 29, 34, 38, 39 |
OC | NGC 2682 | M67 | 0.01 | 2.5 | 0.004 | 4.4 | +0.05 | N | 29, 40, 41 |
OC | NGC 3114 | 0.0016 | 8 | 0.0002 | 0.16 | –0.01 | N | 24, 29, 36, 42 | |
OC | NGC 6134 | 0.0008 | 2 | 0.0004 | 0.7 | + 0.12 | N | 24, 29, 43, 44 | |
OC | NGC 6253 | Melotte 156 | 0.007 | 2 | 0.0035 | 4 | +0.4 | N | 24, 26, 29 |
OC | NGC 6475 | M 7 | 0.007 | 6 | 0.001 | 0.3 | +0.14 | N | 29, 32, 36 |
OC | NGC 6705 | 0.1 | 1.2 | 0.08 | 0.3 | +0.10 | N | 21 | |
OC | NGC 6791 | Berkeley 46 | 0.5 | 5 | 0.1 | 7.5 | +0.30 | N | 29, 45, 46 |
OC | NGC 7789 | Melotte 245 | 0.06 | 5 | 0.01 | 1.6 | +0.04 | N | 29, 36, 41, 47 |
OC | IC 4651 | Melotte 169 | 0.006 | 2 | 0.003 | 1.1 | +0.15 | N | 24, 29, 36, 48 |
Fornax | For 3 | 5.2 | 7.2 | 0.72 | 13 | –2.33 | Y | 49 | |
Fornax | For 5 | 3.2 | 8.5 | 0.38 | 13 | –2.09 | Y | 49 | |
LMC | NGC 1651 | 0.8 | 22 | 0.04 | 1.5 | –0.3 | N | 50, 51, 52 | |
LMC | NGC 1783 | 2.5 | 19 | 0.13 | 1.4 | –0.3 | N | 50, 51, 52 | |
LMC | NGC 1786 | 3.7 | 6.0 | 0.62 | 13 | –1.75 | Y | 53, 54, 55 | |
LMC | NGC 1806 | 1.3 | 15 | 0.08 | 1.4 | –0.3 | N | 50, 56, 57 | |
LMC | NGC 1846 | 1.7 | 15 | 0.11 | 1.4 | –0.3 | N | 50, 56, 58 | |
LMC | NGC 1866 | 0.8 | 19 | 0.04 | 0.2 | –0.3 | N | 50, 59, 60, 61 | |
LMC | NGC 1978 | 2.0 | 8.7 | 0.23 | 2.0 | –0.3 | N | 50, 51, 62, 63, 64, 65 | |
LMC | NGC 2173 | 0.5 | 11 | 0.05 | 1.6 | –0.3 | N | 50, 51, 52 | |
LMC | NGC 2210 | 3.0 | 5.9 | 0.51 | 13 | –1.65 | Y | 53, 54, 55 | |
LMC | NGC 2257 | 2.6 | 19 | 0.14 | 13 | –1.95 | Y | 53, 54, 55 | |
Scutum red supergiant cluster 1 | 0.32 | 2.6 | 0.12 | 0.012 | –0.15 | N | 66, 67 | ||
Scutum red supergiant cluster 2 | 0.40 | 4.6 | 0.087 | 0.017 | –0.15 | N | 66, 67 |
Notes.
Half-mass radii were computed from the half-light radii (apparent size was taken as equivalent to half-light radii) from the literature, assuming a Plummer model for the cluster.
Y: possesses multiple populations; N: multiple populations have been searched for, but not found.
Reference. (1) Carretta et al. (2010); (2) Harris (1996, 2010 edition); (3) Kimmig et al. (2015); (4) Piotto et al. (2015): (5) Lebzelter & Wood (2011); (6) Boyles et al. (2011); (7) Forbes & Bridges (2010); (8) Koleva et al. (2008); (9) Lützgendorf et al. (2013); (10) Mucciarelli et al. (2015); (11) Caloi & D’Antona (2011); (12) Bragaglia et al. (2015) (13) Conroy (2012); (14) Piatek et al. (1994); (15) Zocchi et al. (2012) (16) Mandushev et al. (1991); (17) Lanzoni et al. (2013); (18) Heyl et al. (2012); (19) Miocchi (2007) (20) Villanova et al. (2013); (21) Cantat-Gaudin et al. (2014); (22) Salaris & Weiss (2002); (23) Bragaglia et al. (2012); (24) Tadross (2001) (25) Bragaglia & Tosi (2006) (26) Mikolaitis et al. (2012); (27) Casewell et al. (2014); (28) Lodieu et al. (2014); (29) MacLean et al. (2015); (30) Portegies Zwart et al. (2001) (31) Gebran et al. (2008) (32) Becker & Fenkart (1971); (33) Francic (1989); (34) Reddy et al. (2012); (35) Donati et al. (2014); (36) Gozha et al. (2012); (37) Güneş et al. (2012); (38) Lee et al. (2013); (39) Marconi et al. (1997); (40) Hurley et al. (2005); (41) Pancino et al. (2010); (42) Santrich et al. (2013); (43) Smiljanic et al. (2009) (44) Mikolaitis et al. (2010) (45) Bragaglia et al. (2014) (46) Platais et al. (2011); (47) Wu et al. (2009) (48) Mikolaitis et al. (2011); (49) Larsen et al. (2012); (50) Goudfrooij et al. (2014); (51) Mucciarelli et al. (2008); (52) Niederhofer et al. in prep; (53) Mackey & Gilmore (2003) (54) Mucciarelli et al. (2009); (55) Mucciarelli et al. (2010) (56) Bastian & Niederhofer (2015); (57) Mucciarelli et al. (2014); (58) Mackey et al. (in prep.); (59) Bastian & Silva-Villa (2013); (60) Mucciarelli et al. (2011); (61) Niederhofer et al. (2015); (62) Ferraro et al. (2006); (63) Miloneet al. (2009); (64) Mucciarelli et al. (2007); (65) Werchan & Zaritsky (2011); (66) Davies et al. (2009); (67) Portegies Zwart et al. (2010).
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