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Resolved stellar populations constituting extended UV disks (XUV-disks) in nearby galaxies

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dc.book.titleFormation and evolution of galaxy disks
dc.contributor.authorThilker, D. A.
dc.contributor.authorBianchi, L.
dc.contributor.authorGil De Paz, Armando
dc.contributor.authorMeurer, G.
dc.contributor.authorBoissier, S.
dc.contributor.authorMadore, B. F.
dc.contributor.authorFerguson, A.
dc.contributor.authorHameed, S.
dc.contributor.authorNeff, S.
dc.contributor.authorMartin, C. D.
dc.contributor.authorRich, R. M.
dc.contributor.authorSchiminovich, D.
dc.contributor.authorSeibert, M.;, M.
dc.contributor.authorWyder, T.
dc.contributor.editorFunes, José G.
dc.contributor.editorCorsini, Enrico Maria
dc.date.accessioned2023-06-20T13:43:08Z
dc.date.available2023-06-20T13:43:08Z
dc.date.issued2008
dc.description© Astronomical Society of the Pacific (ASP). International Conference on Formation and Evolution of Galaxy Disks (2007. Rome, Italy). This work was supported by grants HST-GO-10608.01-A and HST-GO-10904.01-A.
dc.description.abstractWe 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.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipThe Space Telescope Science Institute (STScI)
dc.description.sponsorshipNational Aeronautics and Space Administration (NASA)
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/35640
dc.identifier.isbn978-1-58381-662-2
dc.identifier.officialurlhttp://adsabs.harvard.edu/abs/2007arXiv0712.3724T
dc.identifier.relatedurlhttp://adsabs.harvard.edu/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/53489
dc.language.isoeng
dc.page.final224
dc.page.initial223
dc.publication.placeSan Francisco
dc.publisherAstronomical Society of the Pacific (ASP)
dc.relation.ispartofseriesASP Conference Series
dc.relation.projectIDHST-GO-10608.01-A
dc.relation.projectIDHST-GO-10904.01-A
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordAstronomy & Astrophysics
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.titleResolved stellar populations constituting extended UV disks (XUV-disks) in nearby galaxies
dc.typebook part
dc.volume.number396
dcterms.referencesBoissier, S., et al. 2007, ApJS, 173, 524 Ferguson, A., et al. 1998, ApJ, 506, L19 Gil de Paz, A., et al. 2005, ApJ, 627, L29 Thilker, D. A., et al. 2005, ApJ, 619, L79 Thilker, D. A., et al. 2007, ApJS, 173, 538
dspace.entity.typePublication
relation.isAuthorOfPublication7fb1c66f-848a-4aa3-a350-88c633947323
relation.isAuthorOfPublication.latestForDiscovery7fb1c66f-848a-4aa3-a350-88c633947323

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