INFRARED PHOTOMETRY FOR STARS IN THE HYADES MAIN SEQUENCE

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dc.contributor.authorIRIARTE ERRO, B
dc.date.accessioned2026-05-28T16:29:09Z
dc.date.issued1969
dc.description.abstractTaking into account that the Hyades main sequence stars have been used as "standard" stars and provide the basis of comparison with other objects we have obtained infrared colors for them with great precision.
dc.description.paginacion317 -
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent1
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/22317
dc.language.isoInglés
dc.numero.secuencia22314
dc.publisherObservatorio Astrofísico de Tonantzintla, Pue, Pue, Mex
dc.relation.ispartofseriesVol. 5
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectINFRARED PHOTOMETRY, STARS, HYADES, MAIN SEQUENCE
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleINFRARED PHOTOMETRY FOR STARS IN THE HYADES MAIN SEQUENCE
dc.title.alternativeBOL OBS TONAN TACUB

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