We investigate the star cluster system in the starburst galaxy NGC 7673 using archival Hubble Space Telescope WFPC2 broad-band images. For the first time we are able to examine the internal structures of the prominent optical clumps in this galaxy. The clu
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arXiv:astro-ph/0206165v1 11 Jun 2002
Abstract.WeinvestigatethestarclustersysteminthestarburstgalaxyNGC7673usingarchivalHubbleSpaceTelescopeWFPC2broad-bandimages.Forthe rsttimeweareabletoexaminetheinternalstructuresoftheprominentopticalclumpsinthisgalaxy.Theclumpsarecomposedofyoungstars,16 33%ofwhichareinbrightstarclusters.Weidentify268starclustercandidatesinboththeF555WandF814Wimages,and50clusterswiththeF255W lter.Thesedataallowustoestimateagesandmassesusingcolor-magnitudeandtwo-colordiagramsforoursample.We ndapopulationofyoung,<6Myrclus-terslocatedthroughoutthegalaxywithconcentrationsintheclumps.Starclustermassestimatesare5 50×104M⊙forthebrightestobjects.Thestarburstremainsactiveinphysicallywell-separatedregions,indicatingawidespreadstarbursttrigger.Wediscussclumplifetimes,theirimpli-cationsforthefutureevolutionofNGC7673,andpossiblerelationshipstohighredshiftstarbursts.
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