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astro-ph2002
The disruption time of clusters in selected regions of four galaxies
Henny J. G. L. M. Lamers, Stratos G. Boutloukos
If the cluster formation rate is constant and the disruption time of clusters depends on their initial mass as t_dis= t_4 x (M_i/10^4 Msun)^gamma, where M_i is the initial mass of…
astro-ph2002
Star Cluster Formation and Disruption Time-Scales -- I. An empirical determination of the disruption time of star clusters in four galaxies
S. G. Boutloukos, H. J. G. L. M. Lamers
We present a new method to derive the cluster disruption time in selected regions of galaxies from the mass or age distribution of magnitude-limited cluster samples. If the disrupt…