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Table 3:

Values adopted from the literature (Table 2) for the clusters studied in this work, where masses are estimated based on models by Schulz et al. (2002).

Cluster 		Age [ $Z/Z_{\odot}$] log( $M/M_{\odot}$) log( $M/M_{\odot}$)
  (Gyr)   Salpeter Scalo
HW1 5 $\pm$ 1.0 -0.7 $\pm$ -- -- --
K3 6.5 $\pm$ 0.5 -1.2 $\pm$ 0.2 5.0 4.6
L3 1.5 $\pm$ 0.5 -0.7 $\pm$ -- -- --
L11 3.5 $\pm$ 0.5 -0.8 $\pm$ 0.14 4.0 3.7
L113 4.0 $\pm$ 0.7 -1.24 $\pm$ 0.11 -- --
NGC 121 11 $\pm$ 0.5 -1.46 $\pm$ 0.10 5.5 5.2
NGC 152 3.0 $\pm$ 1.0 -1.25 $\pm$ 0.25 4.4 3.9
NGC 222 0.10 $\pm$ 0.03 -0.3 $\pm$ -- 3.8 3.8
NGC 256 0.10 $\pm$ 0.03 -0.3 $\pm$ -- 3.8 3.8
NGC 269 0.3 $\pm$ 0.2 -0.3 $\pm$ -- 4.0 3.8
NGC 294 0.4 $\pm$ 0.2 -0.3 $\pm$ -- 4.4 4.0
NGC 361 6.8 $\pm$ 0.5 -1.45 $\pm$ 0.11 5.1 4.7
NGC 419 1.4 $\pm$ 0.2 -0.3 $\pm$ -- 5.3 4.9
NGC 458 0.13 $\pm$ 0.06 -0.23 $\pm$ -- 3.9 4.2


Source LaTeX | All tables | In the text

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