SAN LUIS POTOSIECTROPHOTOMETRY OF THE ORION NEBULA II THE ABUNDANCE OF ELEMENTS

Simple item page
dc.contributor.authorMENDEZ, ME
dc.date.accessioned2026-05-28T15:54:55Z
dc.date.issued1965
dc.description.abstractUsing a recent spectrophotometric study of the Orion Nebula, the chemical composition of this object is derived. The electron temperature is also given. The abundance by mass is X = 0.713; Y = 0.26 +/- 0.02; Z = 0.027 +/- 0.004, which is very close to the
dc.description.paginacion240 - 245
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent6
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/20852
dc.language.isoInglés
dc.numero.secuencia20849
dc.publisherUNAM, Instituto de Astronomía, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 4
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectSPECTROPHOTOMETRY, ORION NEBULA, II, ABUNDANCE, ELEMENTS
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleSAN LUIS POTOSIECTROPHOTOMETRY OF THE ORION NEBULA II THE ABUNDANCE OF ELEMENTS
dc.title.alternativeBOL OBS TONAN TACUB

Files

Collections

Registros completos