Multi-color observations of Young Star Clusters

Simple item page
dc.creatorAnders, P.
dc.creatorAlvensleben, U. Fritze--v.
dc.creatorde Grijs, R.
dc.date2003-09-04
dc.date.accessioned2026-07-07T02:09:26Z
dc.date.available2026-07-07T02:09:26Z
dc.descriptionWe 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.
dc.description1 page, conference proceeding IAU General Assembly 2003, Sydney, Joint Discussion 06
dc.identifierhttps://arxiv.org/abs/astro-ph/0309155
dc.identifierhttp://arxiv.org/abs/astro-ph/0309155
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6429
dc.subjectAstrophysics
dc.titleMulti-color observations of Young Star Clusters
dc.typetext

Files

Collections

arXiv