BVRI PHOTOELECTRIC PHOTOMETRY FOR 275 STARS LOCATED BETWEEN 25 Y 50

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dc.contributor.authorIRIARTE ERRO, B
dc.date.accessioned2026-05-28T15:56:57Z
dc.date.issued1967
dc.description.abstractBYRI photometry in Johnson's system was done for 275 stars the mayority of which are comprised between -25° and -50°. Due to systematic variations in V magnitude in R. A. of the order of 0.2 magnitude it was decided to use in the present work V magnitudes
dc.description.paginacion33 - 40
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent8
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/21561
dc.language.isoInglés
dc.numero.secuencia21558
dc.publisherObservatorio Astrofísico de Tonantzintla, Pue, Pue, Mex
dc.relation.ispartofseriesVol. 4
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectPHOTOELECTRIC, PHOTOMETRY
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaASTRONOMIA OPTICA
dc.subject.subdisciplinaFOTOELECTRICA
dc.titleBVRI PHOTOELECTRIC PHOTOMETRY FOR 275 STARS LOCATED BETWEEN 25 Y 50
dc.title.alternativeBOL OBS TONAN TACUB

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