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Red Giant Stars in Magellanic Cloud Clusters: Constraining Population Synthesis Models

Published online by Cambridge University Press:  25 May 2016

Léo Girardi
Léo Girardi*
Affiliation:
Max-Planck-Institut für Astrophysik, Garching bei München, Germany

Abstract

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We have developed a population synthesis code, aimed mainly at the interpretation of CMDs. Magellanic Cloud clusters have been largely used for the test/calibration of the underlying stellar tracks.

Type
Part 5. Stellar Populations and Surveys
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 374 - 376
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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