PLANETARY NEBULAE IV PREDICTED CHEMICAL COMPOSITION AND INTERSTELLAR ENRICHMENT

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dc.contributor.authorTORRES PEIMBERT, S
dc.contributor.authorPEIMBERT, M
dc.date.accessioned2026-05-28T16:32:39Z
dc.date.issued1972
dc.description.abstractFor pt. III see abstr. A66513 of 1971. Based on stellar evolution models and on observations of planetary nebulae, the change of chemical abundances in the interstellar medium is studied. It is found that the contribution to the N/O abundance gradient pre
dc.description.paginacion101 - 11
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent1
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/23647
dc.language.isoInglés
dc.numero.secuencia23644
dc.publisherUNAM, Boletín de Observatorios Tonatzintla y Tacubaya, México.
dc.publisherDF
dc.relation.ispartofseriesVol. 6 No. 37
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectPLANETARY, NEBULAE, PREDICTED, CHEMICAL, COMPOSITION, INTERSTELLAR, ENRICHMENT
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titlePLANETARY NEBULAE IV PREDICTED CHEMICAL COMPOSITION AND INTERSTELLAR ENRICHMENT
dc.title.alternativeBOL OBS TONAN TACUB

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