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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
Abstract
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