Chemical evolution of the galactic disk: evidence of an abundance gradient perpendicular to the galactic plane

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.

Guardado en:
Detalles Bibliográficos
Autores principales: Piatti, A.E., Clariá, J.J., Abadi, Mario Gabriel, Mosconi, M.B.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1994
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/159706
Aporte de:
id I19-R120-10915-159706
record_format dspace
spelling I19-R120-10915-1597062024-03-19T15:01:18Z http://sedici.unlp.edu.ar/handle/10915/159706 Chemical evolution of the galactic disk: evidence of an abundance gradient perpendicular to the galactic plane Piatti, A.E. Clariá, J.J. Abadi, Mario Gabriel Mosconi, M.B. 1994 2023-11-02T14:03:15Z es Astronomía Galaxia 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. Asociación Argentina de Astronomía Articulo Comunicacion http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxia
spellingShingle Astronomía
Galaxia
Piatti, A.E.
Clariá, J.J.
Abadi, Mario Gabriel
Mosconi, M.B.
Chemical evolution of the galactic disk: evidence of an abundance gradient perpendicular to the galactic plane
topic_facet Astronomía
Galaxia
description 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.
format Articulo
Comunicacion
author Piatti, A.E.
Clariá, J.J.
Abadi, Mario Gabriel
Mosconi, M.B.
author_facet Piatti, A.E.
Clariá, J.J.
Abadi, Mario Gabriel
Mosconi, M.B.
author_sort Piatti, A.E.
title Chemical evolution of the galactic disk: evidence of an abundance gradient perpendicular to the galactic plane
title_short Chemical evolution of the galactic disk: evidence of an abundance gradient perpendicular to the galactic plane
title_full Chemical evolution of the galactic disk: evidence of an abundance gradient perpendicular to the galactic plane
title_fullStr Chemical evolution of the galactic disk: evidence of an abundance gradient perpendicular to the galactic plane
title_full_unstemmed Chemical evolution of the galactic disk: evidence of an abundance gradient perpendicular to the galactic plane
title_sort chemical evolution of the galactic disk: evidence of an abundance gradient perpendicular to the galactic plane
publishDate 1994
url http://sedici.unlp.edu.ar/handle/10915/159706
work_keys_str_mv AT piattiae chemicalevolutionofthegalacticdiskevidenceofanabundancegradientperpendiculartothegalacticplane
AT clariajj chemicalevolutionofthegalacticdiskevidenceofanabundancegradientperpendiculartothegalacticplane
AT abadimariogabriel chemicalevolutionofthegalacticdiskevidenceofanabundancegradientperpendiculartothegalacticplane
AT mosconimb chemicalevolutionofthegalacticdiskevidenceofanabundancegradientperpendiculartothegalacticplane
_version_ 1807221730389786624