Analysing multi-color observations of young star clusters in mergers

P Anders*, U. Fritze-v. Alvensleben, R de Grijs

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference proceeding contributionpeer-review

Abstract

We 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 ASTROVIRTEL 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''.
Original languageEnglish
Title of host publicationNew horizons in globular cluster astronomy
Subtitle of host publicationproceedings of a conference held at Università di Padova, Padova, Italy 24-28 June, 2002
EditorsGiampaolo Piotto, Georges Meylan, S. George Djougovski, Marco Riello
Place of PublicationSan Francisco, CA
PublisherAstronomical Society of the Pacific
Pages567-568
Number of pages2
ISBN (Print)1583811435
Publication statusPublished - 2003
Externally publishedYes
EventConference on New Horizons in Globular Cluster Astronomy - PADUA, Italy
Duration: 24 Jun 200228 Jun 2002

Publication series

NameAstronomical Society of the Pacific conference series
PublisherAstronomical Society of the Pacific
Volume296

Conference

ConferenceConference on New Horizons in Globular Cluster Astronomy
CountryItaly
CityPADUA
Period24/06/0228/06/02

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