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dc.contributor.authorAnders, P.
dc.contributor.authorFritze, U.
dc.contributor.authorde Grijs, R.
dc.date.accessioned2008-01-30T10:40:33Z
dc.date.available2008-01-30T10:40:33Z
dc.date.issued2003
dc.identifier.citationAnders , P , Fritze , U & de Grijs , R 2003 , Analysing Multi-Color Observations of Young Star Clusters in Mergers . in In: New Horizons in Globular Cluster Astronomy, ASP Conference Proceedings 296 . Astronomical Society of the Pacific , pp. 567-8 .
dc.identifier.isbn1-58381-143-5
dc.identifier.otherdspace: 2299/1467
dc.identifier.urihttp://hdl.handle.net/2299/1467
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/286.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe present a new evolutionary synthesis (ES) tool specifically developed for the analysis of multi-color data of young star clusters (YSCs) in interacting galaxies. Our ESO/ST-ECF ASTROVIRTEL1 project provides an unprecedented database of UV–optical–NIR observations from the HST/WFPC2, HST/NICMOS and VLT data archives. Comparison of these data with ES models for clusters of various metallicities which include gaseous emission as well as various degrees of dust extinction, allows one to independently determine metallicities, ages and extinction for individual clusters. These, in turn, are the basis to derive the mass functions of the YSC systems and to predict the future evolution of their luminosity functions and color distributions. Comparing YSC systems of various ages will, we anticipate, allow us to “see cluster disruption processes at work”.en
dc.format.extent60798
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: New Horizons in Globular Cluster Astronomy, ASP Conference Proceedings 296
dc.titleAnalysing Multi-Color Observations of Young Star Clusters in Mergersen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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