EVOLUTION OF STELLAR MODELS WITH HIGH METAL CONTENT

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dc.contributor.authorTORRES PEIMBERT, S
dc.date.accessioned2026-05-28T16:31:14Z
dc.date.issued1971
dc.description.abstractEvolutionary sequences for stellar configurations between 1 and 1.45 /b M//sub o/ with chemical abundances varying from /b Z/=0.023 to 0.10 and from /b X/=0.60 to 0.68 were computed using the Berkeley Stellar Evolution program. The effect of high metal ab
dc.description.paginacion113 - 30
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent1
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/23140
dc.language.isoInglés
dc.numero.secuencia23137
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.subjectEVOLUTION, STELLAR, MODELS, HIGH, METAL CONTENT
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleEVOLUTION OF STELLAR MODELS WITH HIGH METAL CONTENT
dc.title.alternativeBOL OBS TONAN TACUB

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