Table 2.
Parameters of the clusters used to generate the isochrones and ZAHBs.
| Cluster name | [Fe/H](¶) | Age(¶) | Distance(§) | Distance (adopted) | [α/Fe](&) | Initial mass on HB(@) |
|---|---|---|---|---|---|---|
| (dex) | (Gyr) | (kpc) | (kpc) | (M⊙) | ||
| Arp 2 | −1.45 | 10.9 | 28.6 | 28.6 | 0.31(a) | 0.80 |
| Terzan 8 | −1.80 | 12.2 | 26.7 | 30.0 | 0.37(a) | 0.80 |
| M 54 | −1.25 | 10.7 | 26.7(*) | 26.7 | 0.21(b) | 0.85 |
| Terzan 7 | −0.56 | 7.3 | 22.8 | 22.8 | −0.03(c) | 1.00 |
| NGC 5634 | −1.94 | 11.8 | 27.2 | 27.2 | 0.20(d) | 0.80 |
| NGC 2419 | −2.14 | 12.3 | 83.2 | 100.2 | 0.13(e) | 0.80 |
| NGC 4147 | −1.50 | 12.0 | 18.2 | 19.9 | 0.38(f) | 0.85 |
| Pal 12 | −0.83 | 8.8 | 19.0 | 19.0 | −0.20(g) | 0.90 |
| NGC 6284 | −1.13 | 11.1 | 15.1 | 15.1 | 0.47(h) | 0.90 |
Notes. (¶) from Forbes & Bridges (2010); (§) from Baumgardt et al. (2019); (*)Hamanowicz et al. (2016); (&) the allowed range of [α/Fe] is between 0.0 and 0.3, when the literature value is out of the allowed range, the value closest to the range is selected; (@)Valcarce et al. (2012); (a) Mottini et al. (2008); (b)Brown et al. (1999); (c)Sbordone et al. (2003); (d)Carretta et al. (2017); (e)Sharina et al. (2013); (f)Villanova et al. (2016); (g)Brown et al. (1995); (h)Puzia et al. (2005).
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