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Properties of two star clusters of the LMC: NGC 2164, NGC 1850

Published online by Cambridge University Press:  19 July 2016

A. Vallenari ,
C. Chiosi ,
G. Bertelli ,
G. Meylan  and
S. Ortolani
A. Vallenari
Affiliation:
Department of Astronomy, Padova, Vicolo Osservatorio, 5, Italy Sternwarte, auf dem Hugel 71, Bonn, West Germany
C. Chiosi
Affiliation:
Department of Astronomy, Padova, Vicolo Osservatorio, 5, Italy
G. Bertelli
Affiliation:
Department of Astronomy, Padova, Vicolo Osservatorio, 5, Italy
G. Meylan
Affiliation:
Space Science Institute, Baltimore, USA
S. Ortolani
Affiliation:
Astronomical Observatory, Padova, Vicolo Osservatorio, 5, Italy

Abstract

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We present the photometry of two clusters NGC 2164 and NGC 1850 located in the Large Magellanic Cloud (LMC). The ages are determined taking into account the presence either of convective overshoot or of semiconvection in the stellar models. The experimental luminosity functions are compared with the theoretical models.

Type
Star Formation and Clustering
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 219 - 221
Copyright
Copyright © Kluwer 1991 

References

Bertelli, G., Betto, R., Bressan, A., Chiosi, C., Nasi, E., Vallenari, A. (1990), Astron. Ap. Suppl. in press.Google Scholar
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Vallenari, A., Chiosi, C., Bertelli, G., Meylan, G., Ortolani, S. (1990), Astron. Astrophys. submitted.Google Scholar
Lattanzio, J.C. (1990), UCRL-100283 preprint.Google Scholar