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Globular clusters in the Large Magellanic Cloud: NGC 1866, a test for convective overshoot

C. Chiosi, G. Bertelli, G. Meylan, S. Ortolani

Abstract

La photometrie CCD de l'amas globulaire NGC 1866, du Grand Nuage de Magellan, est presentee. Les fonctions de luminosite et le diagramme magnitude-couleur sont analyses. Un modele d'evolution stellaire de NGC 1866 est developpe. Les resultats numeriques sont compares aux observations

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Key concepts: Physics, Globular cluster, Astrophysics, Large Magellanic Cloud, Stellar evolution, Cepheid variable, Small Magellanic Cloud, Astronomy