INFRARED PHOTOMETRY OF UV CETI STARS

Simple item page
dc.contributor.authorIRIARTE ERRO, B
dc.date.accessioned2026-05-28T16:32:40Z
dc.date.issued1972
dc.description.abstractInfrared photometry is performed on twenty seven M-type dwarf stars, of which nine are stars of the UV Ceti type. The purpose of this study has been to search for infrared excesses in the flare stars. The result of the observations indicates that these st
dc.description.paginacion143 - 147
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent5
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/23650
dc.language.isoInglés
dc.numero.secuencia23647
dc.publisherObservatorio Astrofísico de Tonantzintla, Pue, Pue, Mex
dc.relation.ispartofseriesVol. 6
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectINFRARED, PHOTOMETRY
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleINFRARED PHOTOMETRY OF UV CETI STARS
dc.title.alternativeBOL AGRI

Files

Collections

Registros completos