2026-06-27T10:19:07Zhttps://docta.ucm.es/rest/oai/request

oai:docta.ucm.es:20.500.14352/534892024-09-12T13:08:58Zcom_20.500.14352_14col_20.500.14352_21

Thilker, D. A. Bianchi, L. Gil De Paz, Armando Meurer, G. Boissier, S. Madore, B. F. Ferguson, A. Hameed, S. Neff, S. Martin, C. D. Rich, R. M. Schiminovich, D. Seibert, M.;, M. Wyder, T. 2023-06-20T13:43:08Z 2023-06-20T13:43:08Z 2008 978-1-58381-662-2 https://hdl.handle.net/20.500.14352/53489 http://adsabs.harvard.edu/abs/2007arXiv0712.3724T http://adsabs.harvard.edu/ 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. eng open access Resolved stellar populations constituting extended UV disks (XUV-disks) in nearby galaxies book part