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dc.contributor.authorSilva Villa, Esteban-
dc.contributor.authorKonstantopoulos, I. S.-
dc.contributor.authorSmith, L. J.-
dc.contributor.authorAdamo, A.-
dc.contributor.authorGallagher, J.S-
dc.contributor.authorBastian, N.-
dc.contributor.authorRyon, J. E.-
dc.contributor.authorWestmoquette, M. S.-
dc.contributor.authorZackrisson, E.-
dc.contributor.authorLarsen, S. S.-
dc.contributor.authorWeisz, D. R-
dc.contributor.authorCharlton, J. C.-
dc.date.accessioned2024-06-09T14:08:44Z-
dc.date.available2024-06-09T14:08:44Z-
dc.date.issued2013-
dc.identifier.issn1538-3881-
dc.identifier.urihttps://hdl.handle.net/10495/39816-
dc.description.abstractABSTRACT:We present the Snapshot Hubble U-band Cluster Survey (SHUCS), a project aimed at characterizing the star cluster populations of 10 nearby galaxies (d < 23 Mpc, half within ≈12 Mpc) through new F336W (U-band equivalent) imaging from Wide Field Camera 3, and archival BVI-equivalent data with the Hubble Space Telescope. Completing the UBVI baseline reduces the age–extinction degeneracy of optical colors, thus enabling the measurement of reliable ages and masses for the thousands of clusters covered by our survey. The sample consists chiefly of face-on spiral galaxies at low inclination, in various degrees of isolation (isolated, in group, merging), and includes two active galactic nucleus hosts. This first paper outlines the survey itself, the observational datasets, the analysis methods, and presents a proof-of-concept study of the large-scale properties and star cluster population of NGC 4041, a massive SAbc galaxy at a distance of ≈23 Mpc, and part of a small grouping of six giant members. We resolve two structural components with distinct stellar populations, a morphology more akin to merging and interacting systems. We also find strong evidence of a truncated, Schechter-type mass function, and a similarly segmented luminosity function. These results indicate that binning must erase much of the substructure present in the mass and luminosity functions, and might account for the conflicting reports on the intrinsic shape of these functions in the literature. We also note a tidal feature in the outskirts of the galaxy in Galaxy Evolution Explorer UV imaging, and follow it up with a comprehensive multi-wavelength study of NGC 4041 and its parent group. We deduce a minor merger as a likely cause of its segmented structure and the observed pattern of a radially decreasing star formation rate. We propose that combining the study of star cluster populations with broadband metrics is not only advantageous, but often easily achievable thorough archival datasets.spa
dc.format.extent20 páginasspa
dc.format.mimetypeapplication/pdfspa
dc.language.isoengspa
dc.publisherAmerican Astronomical Society; IOP Publishing.spa
dc.type.hasversioninfo:eu-repo/semantics/publishedVersionspa
dc.rightsinfo:eu-repo/semantics/openAccessspa
dc.rights.urihttp://creativecommons.org/licenses/by/2.5/co/*
dc.titleThe Snapshot Hubble U-band Cluster Survey (SHUCS). I. Survey Description and First Application to the Mixed Star Cluster Population of NGC 4041spa
dc.typeinfo:eu-repo/semantics/articlespa
dc.publisher.groupGrupo de Física y Astrofísica Computacional (FACOM)spa
dc.identifier.doi10.1088/0004-6256/145/5/137-
oaire.versionhttp://purl.org/coar/version/c_970fb48d4fbd8a85spa
dc.rights.accessrightshttp://purl.org/coar/access_right/c_abf2spa
dc.identifier.eissn0004-6256-
oaire.citationtitleAstronomical Journalspa
oaire.citationstartpage1spa
oaire.citationendpage20spa
oaire.citationvolume145spa
oaire.citationissue5spa
dc.rights.creativecommonshttps://creativecommons.org/licenses/by/4.0/spa
dc.publisher.placeWoodbury, Estados Unidosspa
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1spa
dc.type.redcolhttps://purl.org/redcol/resource_type/ARTspa
dc.type.localArtículo de investigaciónspa
dc.subject.lembEncuestas-
dc.subject.lembSurveys-
dc.subject.lembCúmulos de galaxias-
dc.subject.lembGalaxies - Clusters-
dc.subject.lembCúmulos estelares-
dc.subject.lembStars - clusters-
dc.subject.lembGalaxias-
dc.subject.lembGalaxies-
dc.subject.proposalGalaxies: groups: individual (LGG 266)spa
dc.subject.proposalGalaxies: individual (NGC 4041)spa
dc.description.researchgroupidCOL0038262spa
dc.relation.ispartofjournalabbrevAstron. J.spa
Aparece en las colecciones: Artículos de Revista en Ciencias Exactas y Naturales

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