UBV PHOTOELECTRIC PHOTOMETRY FOR FAINT STARS IN THE PLEIADES CLUSTER

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dc.contributor.authorIRIARTE ERRO, B
dc.date.accessioned2026-05-28T16:29:09Z
dc.date.issued1969
dc.description.abstractPhotoelectric photometry in the UBV system of Johnson and Morgan was carried out for 30 stars in the Pleiades Cluster. The main sequence between B-V=+0.6 and +0.8 was found to be very narrow, but from then on a broadening of the main sequence is apparent,
dc.description.paginacion79 - 83
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent5
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/22308
dc.language.isoInglés
dc.numero.secuencia22305
dc.publisherObservatorio Astrofísico de Tonantzintla, Pue, Pue, Mex
dc.relation.ispartofseriesVol. 4
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectUBV, PHOTOELECTRIC, PHOTOMETRY, FAINT STARS, PLEIADES CLUSTER
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleUBV PHOTOELECTRIC PHOTOMETRY FOR FAINT STARS IN THE PLEIADES CLUSTER
dc.title.alternativeBOL OBS TONAN TACUB

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