INFRARED PHOTOMETRY OF V 1057 CYGNI

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dc.contributor.authorMENDOZA, EUGENIO
dc.date.accessioned2026-05-28T16:32:40Z
dc.date.issued1972
dc.description.abstractInfrared and JHKL photometry have been obtained for the extraordinary object V 1057 Cygni at the Observatorio Astronómico Nacional in San Pedro Mártir, Baja California, of Instituto de Astronomia, UNAM. The infrared photometry supports the hypothesis that
dc.description.paginacion135 - 136
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent2
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/23649
dc.language.isoInglés
dc.numero.secuencia23646
dc.publisherUNAM, Instituto de Astronomía, CD MEXICO, DF, 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.disciplinaASTRONOMIA OPTICA
dc.subject.subdisciplinaFOTOMETRIA
dc.titleINFRARED PHOTOMETRY OF V 1057 CYGNI
dc.title.alternativeBOL AGRI

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