The ultraviolet survey of the Gould Belt: general properties of the Taurus star forming region

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dc.contributor.authorGómez De Castro, Ana Inés
dc.contributor.authorLópez Santiago, Javier
dc.contributor.authorSestito, Paola
dc.contributor.authorRodrigo Gudiel, Víctor
dc.contributor.authorLópez Martínez, Fátima
dc.contributor.authorCastro Rubio, Elisa De
dc.contributor.authorCornide, Manuel
dc.contributor.authorYáñez, Javier
dc.date.accessioned2023-06-20T00:13:49Z
dc.date.available2023-06-20T00:13:49Z
dc.date.issued2011-09
dc.description.abstractThe Gould Belt is the local superassociation of star formation. The age of the Belt is some few 10(7) yr, henceforth, its population is dominated by luminous young OB associations and low mass pre-main sequence stars. Attempts to unveil the low mass population have been run making use of the ROSAT all-sky survey. The all sky ultraviolet survey run by the GALaxy Evolution eXplorer (GALEX) maps several regions in the Belt. In this contribution, we present the preliminary analysis of the UV stellar population towards the Taurus region, one of the nearest and best studied regions of star formation.en
dc.description.departmentUnidad Deptal. de Astronomía y Geodesia
dc.description.facultyFac. de Ciencias Matemáticas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Ciencia e Innovación
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/15883
dc.identifier.citationGómez de Castro, A. I., López Santiago, J., Sestito, P. et al. «The Ultraviolet Survey of the Gould Belt: General Properties of the Taurus Star Forming Region». Astrophysics and Space Science, vol. 335, n.o 1, septiembre de 2011, pp. 97-103. DOI.org (Crossref), https://doi.org/10.1007/s10509-011-0687-9.
dc.identifier.doi10.1007/s10509-011-0687-9
dc.identifier.issn0004-640X
dc.identifier.officialurlhttps//doi.org/10.1007/s10509-011-0687-9
dc.identifier.relatedurlhttp://www.springerlink.com/content/v83340108m227704/fulltext.pdf
dc.identifier.urihttps://hdl.handle.net/20.500.14352/42236
dc.issue.number1
dc.journal.titleAstrophysics and space science
dc.language.isoeng
dc.page.final103
dc.page.initial97
dc.publisherSpringer
dc.relation.projectIDAYA2008-06423-C03-01/ESP
dc.rights.accessRightsrestricted access
dc.subject.cdu52
dc.subject.keywordLocal system
dc.subject.keywordMilky-way
dc.subject.keywordCatalog
dc.subject.keywordGas
dc.subject.keywordInstability
dc.subject.keywordEvolution
dc.subject.keywordOrigin
dc.subject.keywordClouds
dc.subject.keywordStar formation
dc.subject.keywordLow mass stars
dc.subject.keywordPre-main sequence stars
dc.subject.keywordStellar populations
dc.subject.ucmAstronomía (Matemáticas)
dc.subject.unesco21 Astronomía y Astrofísica
dc.titleThe ultraviolet survey of the Gould Belt: general properties of the Taurus star forming regionen
dc.typejournal article
dc.volume.number335
dspace.entity.typePublication
relation.isAuthorOfPublication492947a5-78aa-4c19-bb69-3dd332bff97c
relation.isAuthorOfPublicationfac67a6c-a5c6-44e9-a74d-a086abd5aa5f
relation.isAuthorOfPublication.latestForDiscovery492947a5-78aa-4c19-bb69-3dd332bff97c

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