INTERMEDIATE BAND PHOTOMETRY OF V PUPPIS

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dc.contributor.authorMENDOZA, EUGENIO
dc.date.accessioned2026-05-28T16:32:40Z
dc.date.issued1972
dc.description.abstractSome 150 observations were made on V Puppis on the (33, 35, 37, 40, 45, 52, 58, 63)-photometric system. The obtained light curves are of high quality. The observed amplitude of the light variations for the primary minimum depends on the spectral region in
dc.description.paginacion89 - 94
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent6
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/23652
dc.language.isoInglés
dc.numero.secuencia23649
dc.publisherUNAM, Instituto de Astronomía, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 6
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectINTERMEDIATE, BAND, PHOTOMETRY, PUPPIS
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaASTRONOMIA OPTICA
dc.subject.subdisciplinaFOTOMETRIA
dc.titleINTERMEDIATE BAND PHOTOMETRY OF V PUPPIS
dc.title.alternativeBOL AGRI

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