|
1 Introduction
|
|
|
2 The observations
|
|
|
3 Exploration of the parameters which determine the disruption time
|
|
|
4 Input parameters for modeling the cluster population of M 51
|
|
|
5 Analytical model for generating a cluster population
|
|
|
6 Fitting observed age-mass distribution to predictions
|
|
|
7 Implication of the derived disruption time
|
|
|
8 Conclusions
|
|
|
References
|
