Table 2
Adopted cluster parameters.
| Cluster | E(B − V) | (m − M)0 | Age | Rgc | z |
| (mag) | (mag) | (Gyr) | (kpc) | (kpc) | |
|
|
|||||
| Be 26a | 0.68 ± 0.06 | 13.8 ± 0.5 | 4.25 ± 0.25 | 13.9 | 0.24 |
| Be 70b | 0.48 ± 0.10 | 13.1 ± 0.3 | 4.0 ± 0.8 | 12.6 | 0.26 |
| NGC 1798c | 0.51 ± 0.04 | 13.1 ± 0.2 | 1.4 ± 0.3 | 12.5 | 0.35 |
| NGC 2266d | 0.15 ± 0.01 | 12.6 ± 0.2 | 0.7 ± 0.1 | 11.8 | 0.59 |
Notes.
Average of the values by Piatti et al. (2010) and Hasegawa et al. (2008). See text for details.
Values taken from Ann et al. (2002) which are similar to those derived by Hasegawa et al. (2004) with the exception that they derived an age of 2.8 Gyr.
Values taken from Park & Lee (1999) which are similar to others available in the literature within error bars (e.g. Dutra & Bica 2000; Tadross et al. 2002; Salaris et al. 2004; Maciejewski & Niedzielski 2007).
Values taken from Dias et al. (2012). Similar values have been obtained by other investigations in this cluster (Kaluzny & Mazur 1991; Dutra & Bica 2000; Tadross 2001; Tadross et al. 2002; Lata et al. 2002; Salaris et al. 2004; Paunzen & Netopil 2006; Maciejewski & Niedzielski 2007; Maciejewski et al. 2008; Paunzen et al. 2010; Monteiro et al. 2010).
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