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The age distribution function of star clusters in the LMC

Published online by Cambridge University Press:  19 July 2016

M. Alongi  and
C. Chiosi
M. Alongi
Affiliation:
Department of Astronomy, Vicolo dell'Osservatorio 5, I-35122 Padova, Italy
C. Chiosi
Affiliation:
Department of Astronomy, Vicolo dell'Osservatorio 5, I-35122 Padova, Italy

Abstract

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We present the age distribution function for Large Magellanic Cloud (LMC) clusters obtained from a relationship between their integrated U BV colours and age. We discuss further the results by Chiosi et al. (1988) on the nature of the bimodal distribution of the (B - V) colours for LMC clusters. Their conclusion that bimodality in the colour stems from the combined effect of the age distribution function and the rate at which clusters change colour with age, is revisited. The result of our analysis shows that the age distribution is the sole agent and that a real age gap is present. Finally, we draw some conclusions about the efficiency of cluster formation and disruption in the LMC.

Type
Star Formation and Clustering
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 193 - 194
Copyright
Copyright © Kluwer 1991 

References

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