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Resolved Stellar Populations Constituting Extended UV Disks (XUV-disks) in Nearby Galaxies

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arxiv 0712.3724 v1 pith:WDSDIPR2 submitted 2007-12-21 astro-ph

D. A. Thilker , L. Bianchi , G. Meurer , A. Gil de Paz , S. Boissier , B. Madore , A. Ferguson , S. Hameed
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S. Neff C. D. Martin R. M. Rich D. Schiminovich M. Seibert T. Wyder
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classification astro-ph
keywords extendedresolvedadditionanalysisbandsclusteringclusterscomplexes
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We describe HST imaging of recent star formation complexes located in the extended UV disk (XUV-disk) component of NGC 5236 (M 83), NGC 5055 (M 63), and NGC 2090. Photometry in four FUV--visible bands permits us to constrain the type of resolved stars and effective age of clusters, in addition to extinction. The preliminary results given herein focus on CMD analysis and clustering properties in this unique star-forming environment.

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