CHEMICAL ABUNDANCES IN GALACTIC HII REGIONS

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dc.contributor.authorPEIMBERT, M
dc.contributor.authorCOSTERO, R
dc.date.accessioned2026-05-28T16:29:09Z
dc.date.issued1969
dc.description.abstractNew photoelectric observations of Orion, M8, and M17 are presented; from these data the chemical abundances of He, C, N, O, Ne, and S with respect to hydrogen are derived, taking into account the effect of temperature fluctuations over the volumes conside
dc.description.paginacion3 - 22
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent29
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/22316
dc.language.isoInglés
dc.numero.secuencia22313
dc.publisherUNAM, Instituto de Astronomía, CD MEXICO, DF, MEX
dc.publisherUNAM, Instituto de Astronomía, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 5
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectCHEMICAL, ABUNDANCES, GALACTIC, HII, REGIONS
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaGALAXIAS
dc.titleCHEMICAL ABUNDANCES IN GALACTIC HII REGIONS
dc.title.alternativeBOL OBS TONAN TACUB

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