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Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/9193
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dc.contributor.authorParedes i Poy, Josep Mariacat
dc.contributor.authorMartí Ribas, Josepcat
dc.contributor.authorJordi i Nebot, Carmecat
dc.contributor.authorTrullols i Farreny, Enriccat
dc.contributor.authorPeracaula i Bosch, Martacat
dc.date.accessioned2009-08-26T07:28:35Z-
dc.date.available2009-08-26T07:28:35Z-
dc.date.issued1993cat
dc.identifier.issn0365-0138cat
dc.identifier.urihttp://hdl.handle.net/2445/9193-
dc.description.abstractWe present I-band deep CCD exposures of the fields of galactic plane radio variables. An optical counterpart, based on positional coincidence, has been found for 15 of the 27 observed program objects. The Johnson I magnitude of the sources identified is in the range 18-21.eng
dc.format.extent7 p.cat
dc.format.mimetypeapplication/pdfeng
dc.language.isoengeng
dc.publisherEDP Sciencescat
dc.relation.isformatofReproducció digital del document publicat en format paper, proporcionada per NASA Astrophysics Data System http://adsabs.harvard.edu/cat
dc.relation.ispartofAstronomy and Astrophysics Supplement Series, 1993, vol. 102, núm. 2, p. 381-387.cat
dc.rights(c) The European Southern Observatory, 1993cat
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)-
dc.subject.classificationAstrometriacat
dc.subject.classificationProcessament d'imatgescat
dc.subject.otherRadio continuum: generaleng
dc.subject.otherAstrometryeng
dc.subject.otherTechniques: images processingeng
dc.titleOptical counterpart of galactic plane variable radio sourceseng
dc.typeinfo:eu-repo/semantics/articleeng
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec87789cat
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
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