All Tables

Table 1: Comparison of the ZAHB levels, He core masses (in solar mass units), HB evolutionary times (in Myr) and RGB evolutionary times at brighter magnitudes than the ZAHB (in Myr) between the models used in Zoccali et al. (2000), in Paper I, and the models by Cassisi et al. (1998), for two selected metallicities (see text for details).
Table 2: Cluster data. The columns display, respectively, cluster name, measured value of R with associated error, [Fe/H] on the ZW84 and CG97 scale, and value of $HB_{\rm type}$ (see text for details).