P. Anders, U. F. Alvensleben, R. S. U. Goettingen, D. PhysicsAstronomy, U. Sheffield
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We present a new set of evolutionary synthesis models of our GALEV code, specifically developed to include the gaseous emission of presently forming star clusters, in combination with an advanced tool to compare large model grids with multi-color broad-band observations of YSC systems. Tests and first applications are presented.
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