SCYON Abstract

Received on September 8 2003

Multi-color observations of Young Star Clusters

AuthorsPeter Anders (1), Uta Fritze - v. Alvensleben (1), Richard de Grijs (2)
(1) Universitäts-Sternwarte Göttingen, Geismarlandstrasse 11, 37083 Göttingen, Germany,
(2) Department of Physics & Astronomy, The University of Sheffield, Hicks Building, Hounsfield Road, Sheffield S3 7RH, UK
To appear inScientific Highlights of the IAU, IAU XXV, Sydney, Joint Discussion 06


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.