All Tables

Table 1: Observed and theoretical integrated colours for the selected globular clusters. Values from the Harris catalogue are dereddened according to Reed et al. (1988). The J-K near-IR colour is from Brocato et al. (1990a), dereddened according to Cardelli et al. (1989). ${\cal M}/L_V$ is from the compilation by Pryor & Meylan (1993).
Table 2: Integrated colours in the standard UBVRIJHK photometric filters for our standard model with $M_V^{\rm tot}=-8$ and Z=0.0002. (Full version available at CDS.)
Table 3: As in Table 2 but for WFPC2 (first three columns) and NICMOS1 (last two columns) photometric bands. (Full version available at CDS.)
Table 4: The physical ingredients adopted in the models plotted in Fig. 6.
Table 5: Mass-to-light ratios for selected ages in several photometric passbands from our standard model with different assumptions for $M_{\rm up}$ .
Table 6: Theoretical ${\cal M}/L$ as a function of the age in different photometric bands (solar units) obtained for standard models with $M_V^{\rm tot}=-8$ . (Full version available at CDS.)