MULTICOLOR PHOTOMETRY OF LONG PERIOD VARIABLES

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dc.contributor.authorMENDOZA, EUGENIO
dc.date.accessioned2026-05-28T15:56:57Z
dc.date.issued1967
dc.description.abstractMulticolor photometry is made of sixty seven late type stars over wavelengths ranging from 0.3µ to 10.2µ. The observations enable one to distinguish between classes M, S and C. The M and S stars unreddened by interstellar extinction can be separated and t
dc.description.paginacion114 - 148
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent34
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/21560
dc.language.isoInglés
dc.numero.secuencia21557
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 4
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectMULTICOLOR, PHOTOMETRY, LONG PERIOD, VARIABLES
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaASTRONOMIA OPTICA
dc.subject.subdisciplinaFOTOMETRIA
dc.titleMULTICOLOR PHOTOMETRY OF LONG PERIOD VARIABLES
dc.title.alternativeBOL OBS TONAN TACUB

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