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dc.date.accessioned 2023-11-02T14:03:15Z
dc.date.available 2023-11-02T14:03:15Z
dc.date.issued 1994
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/159706
dc.description.abstract Using a revised DDO abundance scale for the galactic open cluster system, the existence and size of the radial and axial abundance gradients, as well as the existence of a global age-metallicity relation in the galactic disk are investigated. en
dc.language es es
dc.subject Galaxia es
dc.title Chemical evolution of the galactic disk: evidence of an abundance gradient perpendicular to the galactic plane en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Piatti, A.E. es
sedici.creator.person Clariá, J.J. es
sedici.creator.person Abadi, Mario Gabriel es
sedici.creator.person Mosconi, M.B. es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 39 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)