Multi-color observations of Young Star Clusters

Details Multi-color observations of Young Star Clusters Multi-color observations of Young Star Clusters

2003-09-04

arxiv.org/abs/astro-ph/0309155v1

Astronomy and Astrophysics

Astrophysics

1 page, conference proceeding IAU General Assembly 2003, Sydney, Joint Discussion 06

Scientific paper

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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