Table 3: Stars in the stellar database. The ages were calculated using the Padova stellar tracks (see text).

Star		 Age (yr)

B0V		 <107
B5-7V 4.4 $\times$ 107
A0V 3.5 $\times$ 108
A5V 4.0 $\times$ 108
F2V 5.7 $\times$ 108
F8V 3.6 $\times$ 109
w F8V 6.5 $\times$ 109
G5V 1.3 $\times$ 1010
w G5V 4.3 $\times$ 109
K2V 4.0 $\times$ 1010
K4V 5.8 $\times$ 1010
M2V >1010
B1-2III 2.8 $\times$ 107
B5III 6.5-10 $\times$ 107
A0III 3 $\times$ 108
A5III 5-6 $\times$ 108
F0III 8.8 $\times$ 108
F5III 1.2-2 $\times$ 109
G0III $\sim $109
G5III 3-4.5 $\times$ 109
w G5III $\sim $109
w G8III $\sim $109
K0III 5.3 $\times$ 109
K3III 6-8.4 $\times$ 109
r K3III 7.5 $\times$ 109
w K3III $\sim $109
K5III 3.4-6.0 $\times$ 109
M5III 3.5-4.5 $\times$ 109
B0I 7 $\times$ 106
B5I 9 $\times$ 106
A0I 1.3 $\times$ 107
A2I 1.3 $\times$ 107
F0I 1.8 $\times$ 107
F8I 2.5 $\times$ 107
G8I 1.5 $\times$ 107
K3I 1.5 $\times$ 107
M2I 4.8 $\times$ 107


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Observations and data reduction
3 Redshift determination and galaxy catalogue
4 Cluster members - definition of the sample and some structural and dynamical properties
5 Stellar population synthesis
6 Analysis on spectral and morphological classes
7 Colours
8 Summary
References
Online Material
List of tables
List of figures