SAN LUIS POTOSIECTROPHOTOMETRY OF THE ORION NEBULA I ON THE NEBULAR STRUCTURE

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dc.contributor.authorMENDEZ, ME
dc.date.accessioned2026-05-28T16:30:13Z
dc.date.issued1970
dc.description.abstractResults of spectrophotometry observations of the Orion Nebula in the wavelength range ? 3600 - 11000 Å are presented. Apparent emission line intensities in various areas of the Huyghenian region have been corrected for interstellar and internebular extinc
dc.description.paginacion91 - 103
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent12
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/22741
dc.language.isoInglés
dc.numero.secuencia22738
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 4
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectSPECTROPHOTOMETRY, ORION NEBULA, NEBULAR STRUCTURE
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaASTRONOMIA OPTICA
dc.subject.subdisciplinaFOTOMETRIA
dc.titleSAN LUIS POTOSIECTROPHOTOMETRY OF THE ORION NEBULA I ON THE NEBULAR STRUCTURE
dc.title.alternativeBOL OBS TONAN TACUB

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