All Tables

Table 1: Clusters sample.
Table 2: Radial velocities plus photometry of the program stars.ID is identification according to Carraro et al. (2005a,b) numbering. The last column indicates whether a star is considered member (M) or not (NM) according to the analysis in Sect. 5.
Table 4: Atmospheric parameters. Typical errors in temperature, logarithm of gravity and micro-turbulent velocity are 100 $^\circ$ K, 0.2 , and 0.1 km s^-1.
Table 5: Mean abundance analysis from cluster members. In parenthesis below the element the number of lines used is indicated.
Table 6: Revision of the fundamental parameters of the clusters under study.
Table 7: Revision of the fundamental parameters of the clusters under study.
Table 8: Additional clusters gathered from the literature. References are: (a) Carraro et al. (2004); (b) Yong et al. (2005); (c) Villanova et al. (2005); (d) Frinchaboy et al. (2007).
Table 3: