All Tables

Table 1: Approximations to the mass lost by stellar evolution for ${\it GALEV}$ cluster models with a Salpeter IMF of $\alpha =-2.35$ , $0.15 < M_* < 85~\mbox{$M_{\odot}$ }$ and 0.0004<Z<0.05.
Table 2: The disruption time and the formation rate of clusters within 600 pc from the Sun for two assumed values of the lower mass limit of clusters in the Kharchenko et al. (2005) sample.