MULTICOLOR PHOTOMETRY OF STELLAR AGGREGATES

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dc.contributor.authorMENDOZA, EUGENIO
dc.date.accessioned2026-05-28T15:58:09Z
dc.date.issued1968
dc.description.abstractWe have made multicolor photometric observations over the range of wavelength from 0.36 microns in the ultraviolet to 5.0 microns in the infrared, on 1063 stars in the regions of h and x Persei, Pleiades, Hyades, Orion, Praesepe M 67, Scorpio-Centaurus, C
dc.description.paginacion149 - 196
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent47
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/21955
dc.language.isoEspañol
dc.numero.secuencia21952
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, STELLAR, AGGREGATES
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleMULTICOLOR PHOTOMETRY OF STELLAR AGGREGATES
dc.title.alternativeBOL OBS TONAN TACUB

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