ON THE S II AND O I LINE INTENSITIES IN GASEOUS NEBULAE AND NUCLEI OF GALAXIES

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dc.contributor.authorPEIMBERT, M
dc.date.accessioned2026-05-28T16:58:45Z
dc.date.issued1979
dc.description.abstractWe present new photoelectric observations of the [S II] line intensities in the nuclei of M51 and M81. It is shown that the [S II]/[O I] line intensity ratios are very similar in objects where the [O I]/[O III] line intensity ratios differ by as much as t
dc.description.paginacion97 - 100
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent4
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/31189
dc.language.isoInglés
dc.numero.secuencia31186
dc.publisherUNAM, Instituto de Astronomía, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 6
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectLINE INTENSITIES, GASEOUS NEBULAE, NUCLEI, GALAXIES
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaGALAXIAS
dc.titleON THE S II AND O I LINE INTENSITIES IN GASEOUS NEBULAE AND NUCLEI OF GALAXIES
dc.title.alternativeBOL AGRI

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