OPACITY FLUCTUATIONS IN THE INTERSTELLAR MEDIUM AT HIGH GALACTIC LATITUDES

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dc.contributor.authorPOVEDA, ARCADIO
dc.date.accessioned2026-05-28T15:53:28Z
dc.date.issued1964
dc.description.abstractInvestigations of the spatial distribution of galaxies by Neyman, Scott and Shane are based on the simplifying assumption that the regions in the sky covered by their work are free from irregular galactic absorption, attributing the observed deviations fr
dc.description.paginacion9 - 15
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent7
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/20472
dc.language.isoEspañol
dc.numero.secuencia20469
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 2 No. 15
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectOPACITY FLUCTUATIONS, INTERSTELLAR MEDIUM, HIGH, GALACTIC LATITUDES
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleOPACITY FLUCTUATIONS IN THE INTERSTELLAR MEDIUM AT HIGH GALACTIC LATITUDES
dc.title.alternativeBOL OBS TONAN TACUB

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