A NOTE ON THE MAGELLANIC CLOUDS

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dc.contributor.authorMENDOZA, EUGENIO
dc.date.accessioned2026-05-28T16:30:13Z
dc.date.issued1970
dc.description.abstractNarrow band photometry has been obtained for 36 stars in the Magellanic Clouds. The observations were calibrated with galactic supergiants to determine the distance to both Clouds. The results for the LMC are excellent, while not so for the SMC. The latte
dc.description.paginacion104 - 106
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent3
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/22744
dc.language.isoInglés
dc.numero.secuencia22741
dc.publisherUNAM, Instituto de Astronomía, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 5
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectNOTE, MAGELLANIC CLOUDS
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaGALAXIAS
dc.titleA NOTE ON THE MAGELLANIC CLOUDS
dc.title.alternativeBOL OBS TONAN TACUB

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